Qyerry Assignment 678910

course Phy202

I think I'm caught good you check please?Thanks

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How do we grades?" "Xɩՙxć

assignment #006

ىjؔަ|

Physics II

06-21-2006

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13:07:54

query introset change in pressure from diameter change given original vel and diameter

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To find the change in pressure when the diameter changes and you know the original velocity. you must first find the new velocity by determining the ratio for the change in diameter and multiplying it be the original velocity. Then calculate the change in pressure by 0.5'rho(v1^2-v2^2).

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13:08:10

** The ratio of velocities is the inverse ratio of cross-sectional areas.

Cross-sectional area is proportional to square of diameter. So velocity is inversely proportional to cross-sectional area:

v2 / v1 = (A1 / A2) = (d1 / d2)^2 so

v2 = (d1/d2)^2 * v1.

Since h presumably remains constant we have

P1 + .5 rho v1^2 = P2 + .5 rho v2^2 so

(P2 - P1) = 0.5 *rho (v1^2 - v2^2) . **

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OK

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13:20:09

query video experiment 4 terminal velocity of sphere in fluid. What is the evidence from this experiment that the drag force increases with velocity?

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13:20:40

** When weights were repetitively added the velocity of the sphere repetively increased. As the velocities started to aproach 0.1254 m/sec the added weights had less and less effect on increasing the velocity. We conclude that as the velocity increased so did the drag force of the water. **

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My exp. Vidoes aren't working for 1-14

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13:20:51

query univ phy problem 14.85 (14.89 10th edition) half-area constriction then open to outflow at dist h1 below reservoir level, tube from lower reservoir into constricted area, same fluid in both. Find ht h2 to which fluid in lower tube rises.

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G-PHY

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13:20:58

** The fluid exits the narrowed part of the tube at atmospheric pressure. The widened part at the end of the tube is irrelevant--it won't be filled with fluid. So Bernoulli's Equation will tell you that the fluid velocity in this part is vExit such that .5 rho vExit^2 = rho g h1.

Now compare three points: point 1, in the narrowed tube; point 2 at the top of the fluid in the lower tube; and point 3 at the level of the fluid surface in the lower container.

At point 1 the pressure is atmospheric and velocity is vExit. Pressure is atmospheric because there is no pressure loss within the tube, since friction and viscosity are both assumed negligible.

At point 2 fluid velocity is zero and since there is no fluid between the narrowed tube and this point there is no net rho g h contribution to Bernoulli's equation. So we have .5 rho v1^2 + P1 = .5 rho v2^2 + P2. P1 is atmospheric and v1 is vExit from above, while v2 = 0 so P2 = atmospheric pressure + .5 rho vExit^2 = atmospheric pressure + rho g h1.

Now comparing point 2 with point 3 we see that there is a difference h in the fluid altitude, with velocity 0 at both points and atmospheric pressure at point 3. Thus P2 + rho g h2 = P3 + rho g h3, or (atmospheric pressure + rho g h1) + rho g h2 = atmospheric pressure + rho g h3. Thus rho g (h3 - h2) = rho g h1 and h3 - h2, which is the height of the fluid in the lower tube, is just equal to h1.

If we assume that somehow the fluid manages to expand on escaping the narrowed tube so that it fills the once-again-widened tube, and exits with vExit as above, then the velocity in the narrowed tube will be 2 * vExit. This leads to the conclusion that pressure change from small to large tube is .5 rho (2 vExit)^2 - .5 rho vExit^2 = .5 rho (3 vExit^2). Since pressure is atmospheric in the large tube, pressure in the small tube is atmospheric pressure + 3 ( .5 rho vExit^2). If we use this pressure for point 1 and follow the steps given above we conclude that h3 - h2, the height of the fluid column in the lower tube, is 3 h1. This is the book's answer. Again I don't have the problem in front of me and I might have missed something, but the idea of the fluid expanding to refill the larger pipe doesn't seem consistent with the behavior of even ideal liquids, which are pretty much incompressible at ordinary pressures. However note that I am sometimes wrong when I disagree with the textbook's solution. **

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G-PHY

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13:21:07

query univ phy problem 14.85 (14.89 10th edition) half-area constriction then open to outflow at dist h1 below reservoir level, tube from lower reservoir into constricted area, same fluid in both. Find ht h2 to which fluid in lower tube rises.

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RESPONSE -->

G-PHY

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13:21:19

** The fluid exits the narrowed part of the tube at atmospheric pressure. The widened part at the end of the tube is irrelevant--it won't be filled with fluid. So Bernoulli's Equation will tell you that the fluid velocity in this part is vExit such that .5 rho vExit^2 = rho g h1.

Now compare three points: point 1, in the narrowed tube; point 2 at the top of the fluid in the lower tube; and point 3 at the level of the fluid surface in the lower container.

At point 1 the pressure is atmospheric and velocity is vExit. Pressure is atmospheric because there is no pressure loss within the tube, since friction and viscosity are both assumed negligible.

At point 2 fluid velocity is zero and since there is no fluid between the narrowed tube and this point there is no net rho g h contribution to Bernoulli's equation. So we have .5 rho v1^2 + P1 = .5 rho v2^2 + P2. P1 is atmospheric and v1 is vExit from above, while v2 = 0 so P2 = atmospheric pressure + .5 rho vExit^2 = atmospheric pressure + rho g h1.

Now comparing point 2 with point 3 we see that there is a difference h in the fluid altitude, with velocity 0 at both points and atmospheric pressure at point 3. Thus P2 + rho g h2 = P3 + rho g h3, or (atmospheric pressure + rho g h1) + rho g h2 = atmospheric pressure + rho g h3. Thus rho g (h3 - h2) = rho g h1 and h3 - h2, which is the height of the fluid in the lower tube, is just equal to h1.

If we assume that somehow the fluid manages to expand on escaping the narrowed tube so that it fills the once-again-widened tube, and exits with vExit as above, then the velocity in the narrowed tube will be 2 * vExit. This leads to the conclusion that pressure change from small to large tube is .5 rho (2 vExit)^2 - .5 rho vExit^2 = .5 rho (3 vExit^2). Since pressure is atmospheric in the large tube, pressure in the small tube is atmospheric pressure + 3 ( .5 rho vExit^2). If we use this pressure for point 1 and follow the steps given above we conclude that h3 - h2, the height of the fluid column in the lower tube, is 3 h1.

This is the book's answer. Again I don't have the problem in front of me and I might have missed something, but the idea of the fluid expanding to refill the larger pipe doesn't seem consistent with the behavior of liquids, which are pretty much incompressible at ordinary pressures. However note that I am sometimes wrong when I disagree with the textbook's solution. **

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G-PHY

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Fy|tz{o߱ͳ∗G~

assignment #007

ىjؔަ|

Physics II

06-21-2006

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13:46:49

Query set 5 problems 16-20

explain how we calculate the average force exerted by a particle of mass m moving at speed v which collides at a time interval `dt elastically and at a right angle with a solid wall

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RESPONSE -->

The average force is equal to the average rate of momentum change. Which is equal to the momentum change divided by the 'dt. The momentum change is found by multiplying velocity by the mass of the particle.

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13:49:17

** The impulse exerted on a particle in a collision is the change in the momentum of that particle during a collision.

The impulse-momentum theorem says that the change in momentum in a collision is equal to the impulse, the average force * the time interval between collisions.

The average force is thus change in momentum / time interval; the time interval is the round-trip distance divided by the velocity, or 2L / v so the average force is -2 m v / ( 2L / v) = m v^2 / L

If there were N such particles the total average force would be N * m v^2 / L

If the directions are random we distribute the force equally over the 3 dimensions of space and for one direction we get get 1/3 the force found above, or 1/3 N * m v^2 / L.

This 3-way distribution of force is related to the fact that for the average velocity vector we have v^2 = vx^2 + vy^2 + vz^2, where v is average magnitude of velocity and vx, vy and vz the x, y and z components of the velocity (more specifically the rms averages--the square root of the average of the squared components). **

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Ok I understand

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13:52:11

Summarize the relationship between the thermal energy that goes into the system during a cycle, the work done by the system during a cycle, and the thermal energy removed or dissipated during the cycle.

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The thernal energy going into a system has to equal the work done by the system plus the thermal enegy dissipated by the system. The less thermal energy dissipated during the cycle the efficient the systme is

e=W/Qin

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13:52:20

** Work-energy is conserved within an isolated system. So the thermal energy that goes into the system must equal the total of the work done by the system and the thermal energy removed from the system. What goes in must come out, either in the form of work or thermal energy. **

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Yes

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13:56:21

If you know the work done by a thermodynamic system during a cycle and the thermal energy removed or dissipated during the cycle, how would you calculate the efficiency of the cycle?

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The efficiency of the system is the ratio of work done and thermal energy going into the system. The thermal energy going in is equal to Work +Qout. So if you add these two together and divide by the work done you'll have the efficiency of the system

e=W/Qin=W/(W+Qout)

or e= (Qin-Qout/Qin)

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13:56:34

** STUDENT SOLUTION: Efficiency is work done / energy input. Add the amount thermal energy removed to the amount of work done to get the input. Then, divide work by the energy input. **

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Yes

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13:59:25

prin phy and gen phy problem 15.2, cylinder with light frictionless piston atm pressure, 1400 kcal added, volume increases slowly from 12.0 m^3 to 18.2 m^3. Find work and chagne in internal energy.

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When 1400kcal of heat is added to gas in a piston at atm, the volume is observed to increase slowly from 12.0m^3 to 18.2m^3. Calculate (a) the work done by the gas, and (b) the change in internal energy of the gas.

Thus 'dV=6.2m^3 and Q=1400kcal(4.186x10^3)=5.86x10^6J

(a)W=P'dV= (1.013x10^3)(6.2m^3)=6.28x10^5J

(b)'dU=Q-W so 'dU=5.86x10^6J-6.28x10^5J=5.232x10^6J

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13:59:52

Work done at constant pressure is P `dV, so the work done in this situation is

`dW = P `dV = 1 atm * (18.2 m^3 - 12 m^3) = (101.3 * 10^3 N/m^2) * (6.2 m^3) = 630 * 10^3 N * m = 6.3 * 10^5 J.

A total of 1400 kcal = 1400 * 4200 J = 5.9 * 10^6 J of thermal energy is added to the system, the change in internal energy is

`dU = `dQ - `dW = 5.9*10^6 J - 6.3 * 10^5 J = 5.9 * 10^6 J - .63 * 10^6 J = 5.3 * 10^6 J.

It is worth thinking about the P vs. V graph of this process. The pressure P remains constant at 101.3 * 10^3 J as the volume changes from 12 m^3 to 18.2 m^3, so the graph will be a straight line segment from the point (12 m^3, 101.3 * 10^3 J) to the point (18.2 m^3, 101.3 * 10^3 J). This line segment is horizontaland the region above the horizontal axis and beneath the segment is a rectangle whose width is 6.2 * 10^3 m^3 and whose altitude is 101.3 * 10^3 N/m^2; its area is therefore the product of its altitude and width, which is 6.3 * 10^5 N m, or 6.3 * 10^5 J, the same as the word we calculated above.

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RESPONSE -->

Sounds good to me

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14:06:44

prin phy and gen phy problem 15.5, 1.0 L at 4.5 atm isothermally expanded until pressure is 1 atm then compressed at const pressure to init volume, final heated to return to original volume. Sketch and label graph.

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The graph has the Pressure on the vertical (y) axis and the Volume on the horizonatal (x) axis. From top to bottom the pressure shows 4.5atm down to 1 atm and from left to right the volume changes form 1 to 4.5L.

There is a slope concave line from 4.5atm to 4.5L representing the Isothermal expansion, and a striaght line from 4.5L to 1L repesenting the Isobaric compression

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14:08:16

When a confined ideal gas is expanded isothermally its pressure and volume change, while the number of moled and the temperature remain constant. Since PV = n R T, it follows that P V remains constant.

In the initial state P = 4.5 atm and V = 1 liter, so P V = 4.5 atm * 1 liter = 4.5 atm * liter (this could be expressed in standard units since 1 atm = 101.3 kPa = 101.3 * 10^3 N/m^2 and 1 liters = .001 m^3, but it's more convenient to first sketch and label the graph in units of atm and liters). During the isothermal expansion, therefore, since P V remains constant we have

P V = 4.5 atm liters. At a pressure of 1 atm, therefore, the volume will be V = 4.5 atm liter / P = 4.5 atm liter / (1 atm) = 4.5 liters.

The graph follows a curved path from (1 liter, 4.5 atm) to (4.5 liters, 1 atm).

At the gas is compressed at constant pressure back to its initial 1 liter volume, the pressure remains constant so the graph follows a horizontal line from (4.5liters, 1 atm) to (1 liter, 1 atm). Note that this compression is accomplished by cooling the gas, or allowing it to cool.

Finally the gas is heated at constant volume until its pressure returns to 4.5 atm. The constant volume dictates that the graph follow a vertical line from (1 liter, 1 atm) back to (4.5 liters, 1 atm).

The graph could easily be relabeled to usestandard metric units.

1 atm = 101.3 kPa = 101.3 * 10^3 Pa = 101.3 * 10^3 N/m^2, so

4.5 atm = 4.5 * 101.3 * 10^3 Pa = 4.6 * 10^3 Pa = 4.6 * 10^3 N/m^2.

1 liter = .001 m^3 so 4.5 liters = 4.5 m^3.

Since P V = 4.5 atm liters, P = 4.5 atm liters / V. This is of the form P = c / V, with c a constant. For positive values of V, this curve descendsfrom a vertical asymptote with the vertical axis (the V axis) through the point (1, c) then approaches a horizontal asymptote with the horizontal axis. For c = 4.5 atm liters, the curve therefore passes through the point (1 liter, 4.5 atm). As we have seen it also passes through (4.5 liters, 1 atm).

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RESPONSE -->

I left out the portion for the IsoVolmetric change from 1atm to 4.5atm because the querry question did not ask for it, it was included in my HW that was turned in.

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14:13:49

gen phy problem 15.12, a-c curved path `dW = -35 J, `dQ = -63 J; a-b-c `dW = - 48 J

gen phy how much thermal energy goes into the system along path a-b-c and why?

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a-c, W=-35J, Q=-63J

a-b-c, W=-48J

a)What is Q for path a-b-c? Qabc=(-48J)

b)If Pa=0.5Pb, what is W for c-d-a? W= 48J

c)What is Q for c-d-a? Q= 48J

d)What is Ua-Uc? 'dU=(-63J-(-35J))=-28J

e)If Ud-Uc=5J, what is Q for d-a? W=0, Q='dU =5J

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E|Đҗl}}

assignment #007

ىjؔަ|

Physics II

06-21-2006

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14:20:26

Query set 5 problems 16-20

explain how we calculate the average force exerted by a particle of mass m moving at speed v which collides at a time interval `dt elastically and at a right angle with a solid wall

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RESPONSE -->

I've already don the section as I was working thu this querry I clicked on diplay notes and it crashed. I'll pick up whrer I left off. I had just finished 15-12 text question

I'll delete the interim for you

OK we're back we it crashed.

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14:31:13

gen phy How are the work done by the system, the thermal energy added to the system and the change in the internal energy of the system related, and what is this relationship have to do with conservation of energy?

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The thermal energy added to the system must equal the work performed and thethermal energy dissipated by the system.

conservation of energy states that the energy in must equal the energy out. Which the energy out is the Work plus the energy dissipated.

As for as the change in internal energy, if work is done by the system the internal energy is reduced if the work is done on the system the internal energy will increase.

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14:31:38

** If a system does work it tends to reduce internal energy, so `dW tends to decrease `dU. If thermal energy is added to the system `dQ tends to increase `dU. This leads to the conclusion that `dU = `dQ - `dW. Thus for example if `dW = -48 J and `dU = -28 J, `dQ = `dU + `dW = -28 J + -48 J = -76 J. **

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This basically what I said

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14:36:54

gen phy How does the halving of pressure caused a halving of the magnitude of the work, and why is the work positive instead of negative as it was in the process a-b-c?

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Well I'm not sure what a-b-c is referenced to but Work is equal to Force times distance or Pressure times 'dV,

Work will be positive is the work is performed on the system and negitive if its done by the system

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14:38:00

** Work is the area under the pressure vs. volume curve. If you have half the pressure between two volumes the graph has half the altitude, which leads to half the area.

The 'width' of a region is final volume - initial volume. If the direction of the process is such that final volume is less than initial volume (i.e., going 'backwards', in the negative x direction) then with 'width' is negative and the area is negative. **

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OK I thought we were referring to the same curve but wasn't sure. Then expanding on what I said it makes sence

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14:38:35

.

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I clicked Next question now I see nothing, I'll try again

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14:38:48

query univ phy problem 19.56 (17.40 10th edition) compressed air engine, input pressure 1.6 * 10^6 Pa, output 2.8 * 10^5 Pa, assume adiabatic.

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G_PHY

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14:39:03

** For an adiabatic process in an ideal gas you know that PV = nRT and PV^`gamma is constant.

You are given P1 and P2, and you want T2 > 273 K to prevent formation of frost.

Assume T2 = P2 V2 / (n R) = 273 K and n R = (P2 V2) / 273 K .

Then T1 = P1 V1 / (n R) = P1 V1 * 273 K / (P2 V2) = (P1 / P2) * (V1 / V2) * 273 K.

Since PV^`gamma = constant it follows that V1 / V2 = (P2 / P1)^(1/`gamma) = (P1 / P2)^(-1/`gamma).

Thus T1 = (P1 / P2) ( P1 / P2)^(-1/`gamma) * 273 K = (P1 / P2)^(1 - 1/`gamma) = (P1 / P2)^(1-1/1.4) * 273 K = (P1 / P2)^.29 * 273 K = 5.6^.29 * 273 K = 443 K, approx. **

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G_PHY

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14:39:09

query univ 19.62 (17.46 10th edition) .25 mol oxygen 240 kPa 355 K. Isobaric to double vol, isothermal back, isochoric to original pressure.

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G_PHY

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14:39:18

** .25 mol oxygen at 240 kPa occupies about V = n R T / P = .25 mol * 8.31 J / (mol K) * 355 K / (2.4 * 10^5 N/m^2) = .003 m^3, very approximately.

Doubling volume, `dV = 2 * V - V = V = .003 m^2 and P = 2.4 * 10^5 Pa so P `dv = 700 J, very approximately.

During isothermal compression we have n = const and T = const so P = n R T / V. Compressing to half the volume, since PV = const, gets us to double the pressure, so max pressure is 2 * 240 kPA = 480 kPa.

To get work we integrate P dV. Integral of P dV is calculated from antiderivative n R T ln | V |; integrating between V1 and V2 we have n R T ln | V2 | - n R T ln | V1 | = n R T ln | V2 / V1 |. In this case V2 = V and V1 = 2 V so V2 / V1 = 1/2 and we have `dW = n R T ln(1/2) = .25 mol * 8.31 J/(mol K) * 710 K * (-.7) = -1000 J, approx.

So net work is about 700 J - 1000 J = -300 J **

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RESPONSE -->

G_PHY

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14:39:24

univ phy describe your graph of P vs. V

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RESPONSE -->

G_PHY

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14:39:29

** The graph proceeds horizontally to the right from original P and V to doubled V, then to the left along a curve that increases at an incr rate as we move to the left (equation P = 2 P0 V0 / V) until we're just above the starting point, then vertically down to the starting pt. **

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RESPONSE -->

G_PHY

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14:39:35

univ phy What is the temperature during the isothermal compression?

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G_PHY

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14:39:40

** If vol doubles at const pressure then temp doubles to 710 K, from which isothermal compression commences. So the compression is at 710 K. **

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RESPONSE -->

G_PHY

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14:39:45

univ phy What is the max pressure?

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RESPONSE -->

G_PHY

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14:39:49

** It starts the isothermal at the original 240 kPa and its volume is halved at const temp. So the pressure doubles to 480 kPa. **

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RESPONSE -->

G_PHY

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۟v爙؅

assignment #008

ىjؔަ|

Physics II

06-21-2006

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14:46:29

prin phy and gen phy problem 15.19 What is the maximum efficiency of a heat engine operating between temperatures of 380 C and 580 C?

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What is the maximum efficiency of a heat engine whose operating temperatures are 580*C(853K) and 380*C(653K)?

eideal =1-(TL/TH)=1-(653K/853K)=.2345=23.45%

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14:46:42

The maximum possible efficiency is (T_h - T_c) / T_h, where T_h and T_c are the absolute max and min operating temperatures.

T_h is (580 + 273)K = 853 K and T_c is (380 + 273) K = 653 K, so the maximum theoretical efficiency is

max efficiency = (T_h - T_c) / T_h = (853 K - 653 K) / (853 K) = .23, approx.

This means that the work done by this engine will be not greater than about 23% of the thermal energy that goes into it.

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Yes

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14:47:50

query gen phy problem 15.26 source 550 C -> Carnot eff. 28%; source temp for Carnot eff. 35%?

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A heat engine utilizes a heat source at 550*C and has an ideal (Carnot) efficiency of 28%. To increase the efficiency to 35% what must be the new temperature of the heat source?

eideal=1-(TL/TH)

.28=1-(TL/823K)

TL=(1-e)( TH)=592.6K

TH= TL /(1-.28) is held constant so the new TH

The new TH is TH= TL /(1-.35) and since is held constant

TH-New= TL/(1-.35)= 592.6K/(1-.35)=911.54K or 638.54*C

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14:48:08

** Carnot efficiency is eff = (Th - Tc) / Th.

Solving this for Tc we multiply both sides by Th to get

eff * Th = Th - Tc so that

Tc = Th - eff * Th = Th ( 1 - eff).

We note that all temperatures must be absolute so we need to work with the Kelvin scale (adding 273 C to the Celsius temperature to get the Kelvin temperature)

If Th = 550 C = 823 K and efficiency is 30% then we have

Tc =823 K * ( 1 - .28) = 592 K.

Now we want Carnot efficiency to be 35% for this Tc. We solve eff = (Th - Tc) / Th for Th:

Tc we multiply both sides by Th to get

eff * Th = Th - Tc so that

eff * Th - Th = -Tc and

Tc = Th - eff * Th or

Tc = Th ( 1 - eff) and

Th = Tc / (1 - eff).

If Tc = 576 K and eff = .35 we get

Th = 592 K / ( 1 - .35 ) = 592 C / .6 = 912 K, approx.

This is (912 - 273) C = 639 C. **

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RESPONSE -->

Yes

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14:48:20

univ phy problem 20.44 (18.40 10th edition) ocean thermal energy conversion 6 C to 27 C

At 210 kW, what is the rate of extraction of thermal energy from the warm water and the rate of absorption by the cold water?

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G-PHY

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14:48:23

** work done / thermal energy required = .07 so thermal energy required = work done / .07.

Translating directly to power, thermal energy must be extracted at rate 210 kW / .07 = 30,000 kW. The cold water absorbs what's left after the 210 kW go into work, or 29,790 kW.

Each liter supplies 4186 J for every degree, or about 80 kJ for the 19 deg net temp change. Needing 30,000 kJ/sec this requires about 400 liters / sec, or well over a million liters / hour.

Comment from student: To be honest, I was suprised the efficiency was so low.

Efficiency is low but the energy is cheap and environmental impact in the deep ocean can be negligible so the process can be economical, if a bit ugly. **

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G-PHY

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DOwѕ螳ͭ

assignment #009

ىjؔަ|

Physics II

06-21-2006

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14:54:25

Query introductory set 6, problems 1-10

explain how we know that the velocity of a periodic wave is equal to the product of its wavelength and frequency

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RESPONSE -->

Since the frequency is how many peak-to-peak cycles of the travelling wave has past in a unit of time and the wave length is the distance between the peaks we can find the velocity, which is distance traveled in a unit of time, by multiplying frequency by the wavelength

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14:54:43

** we know how many wavelength segments will pass every second, and we know the length of each, so that multiplying the two gives us the velocity with which they must be passing **

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RESPONSE -->

In a more general statement Yes

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14:54:48

** we know how many wavelength segments will pass every second, and we know the length of each, so that multiplying the two gives us the velocity with which they must be passing **

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RESPONSE -->

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14:58:45

explain how we can reason out that the period of a periodic wave is equal to its wavelength divided by its velocity

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RESPONSE -->

The period, time required for one cylce of a periodic wave is the inverse of its frequency, the cycles per second.

So if v=f*Wavelength, and T=1/f, and f=velocity/wavelength

Then

T=wavelength/velocity

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14:58:59

** If we know how far it is between peaks (wavelength) and how fast the wavetrain is passing (velocity) we can divide the distance between peaks by the velocity to see how much time passes between peaks at a given point. That is, period is wavelength / velocity. **

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RESPONSE -->

Yes

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15:16:34

explain why the equation of motion at a position x along a sinusoidal wave is A sin( `omega t - x / v) if the equation of motion at the x = 0 position is A sin(`omega t)

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RESPONSE -->

The x/v is the time lag distance/velocity, and sonce distance is zero, x=0 (refernce point) the equation simplifies to

A sin(`omega t)

The time lag is the time required for the wave to propagate from x = 0 to some.

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15:17:12

** the key is the time delay. Time for the disturbance to get from x = 0 to position x is x / v. What happens at the new position is delayed by time x/v, so what happens there at clock time t happened at x=0 when clock time was t = x/v.

In more detail: If x is the distance down the wave then x / v is the time it takes the wave to travel that distance. What happens at time t at position x is what happened at time t - x/v at position x=0.

That expression should be y = sin(`omega * (t - x / v)).

}

The sine function goes from -1 to 0 to 1 to 0 to -1 to 0 to 1 to 0 ..., one cycle after another. In harmonic waves the motion of a point on the wave (think of the motion of a black mark on a white rope with vertical pulses traveling down the rope) will go thru this sort of motion (down, middle, up, middle, down, etc.) as repeated pulses pass.

If I'm creating the pulses at my end, and that black mark is some distance x down in rope, then what you see at the black mark is what I did at time x/v earlier. **

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RESPONSE -->

A lot more detailed but the same result

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15:26:59

Query introductory set six, problems 11-14

given the length of a string how do we determine the wavelengths of the first few harmonics?

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RESPONSE -->

The wavelength is the time it would take for a wave to travel down the string and back, so the wavelength would be 2*L of the string.

'lambda=2L for its fundamental frequency.

Then for the first 3 harmonis, 2nd, 3rd and 4th harmonics we would have 2,3,4 half wavelengths.

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15:27:11

** As wavelength decreases you can fit more half-waves onto the string. You can fit one half-wave, or 2 half-waves, or 3, etc..

So you get

1 half-wavelength = string length, or wavelength = 2 * string length; using `lambda to stand for wavelength and L for string length this would be

1 * 1/2 `lambda = L so `lambda = 2 L.

For 2 wavelengths fit into the string you get

2 * 1/2 `lambda = L so `lambda = L.

For 3 wavelengths you get

3 * 1/2 `lambda = L so `lambda = 2/3 L; etc.

}

Your wavelengths are therefore 2L, L, 2/3 L, 1/2 L, etc.. **

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RESPONSE -->

yes

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15:31:07

Given the wavelengths of the first few harmonics and the velocity of a wave disturbance in the string, how do we determine the frequencies of the first few harmonics?

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RESPONSE -->

The harmonic frequencies are multiples of the fundemental frequency which is equal to the velocity divided by the wavelength. So you could find the funemental frequency and multiply it bey 2,3, and 4 for the 2nd, 3rd, and 4th harmonic frequency.

Or take the velocity and divide it by the wavelength for that harmonic and find the frequency

f=v/'lambda

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15:31:17

** The frequency is the number of crests passing per unit of time.

We can imagine a 1-second chunk of the wave divided into segments each equal to the wavelength. The number of peaks is equal to the length of the entire chunk divided by the length of a 1-wavelength segment. This is the number of peaks passing per second.

So frequency is equal to the wave velocity divided by the wavelength. **

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RESPONSE -->

Yes sir

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15:34:48

Given the tension and mass density of a string how do we determine the velocity of the wave in the string?

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RESPONSE -->

The velocity of the string can be found by dividing the tension by the mass density and taking the square root of the result because

v='sqrt(Ft/(m/L))

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15:35:01

** We divide tension by mass per unit length and take the square root:

v = sqrt ( tension / (mass/length) ). **

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RESPONSE -->

Yes

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15:40:50

gen phy explain in your own words the meaning of the principal of superposition

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RESPONSE -->

Superposition is when two waves travelling in opposite direction meet and there displacements (amplitude and phase) are summed together to form a new wave at this point.

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15:41:05

** the principle of superposition tells us that when two different waveforms meet, or are present in a medium, the displacements of the two waveforms are added at each point to create the waveform that will be seen. **

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RESPONSE -->

Says the same thing

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15:44:45

gen phy what does it mean to say that the angle of reflection is equal to the angle of incidence?

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RESPONSE -->

It means that a when a wave hits something in its path the angle at which it struck the object will be the same as the angle of the reflected wave.

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15:44:53

** angle of incidence with a surface is the angle with the perpendicular to that surface; when a ray comes in at a given angle of incidence it reflects at an equal angle on the other side of that perpendicular **

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RESPONSE -->

Yes

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{ᄞy˃M^R|

assignment #010

ىjؔަ|

Physics II

06-21-2006

"

Your work on this assignment is very good. Let me know if you have questions.

Qyerry Assignment 678910

course Phy202

I think I'm caught good you check please?Thanks

Your work has been received. Please scroll through the document to see any inserted notes (inserted at the appropriate place in the document, in boldface) and a note at the end. The note at the end of the file will confirm that the file has been reviewed; be sure to read that note. If there is no note at the end, notify the instructor through the Submit Work form, and include the date of the posting to your access page.

How do we grades?" "Xɩՙxć

assignment #006

ىjؔަ|

Physics II

06-21-2006

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13:07:54

query introset change in pressure from diameter change given original vel and diameter

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RESPONSE -->

To find the change in pressure when the diameter changes and you know the original velocity. you must first find the new velocity by determining the ratio for the change in diameter and multiplying it be the original velocity. Then calculate the change in pressure by 0.5'rho(v1^2-v2^2).

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13:08:10

** The ratio of velocities is the inverse ratio of cross-sectional areas.

Cross-sectional area is proportional to square of diameter. So velocity is inversely proportional to cross-sectional area:

v2 / v1 = (A1 / A2) = (d1 / d2)^2 so

v2 = (d1/d2)^2 * v1.

Since h presumably remains constant we have

P1 + .5 rho v1^2 = P2 + .5 rho v2^2 so

(P2 - P1) = 0.5 *rho (v1^2 - v2^2) . **

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RESPONSE -->

OK

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13:20:09

query video experiment 4 terminal velocity of sphere in fluid. What is the evidence from this experiment that the drag force increases with velocity?

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RESPONSE -->

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13:20:40

** When weights were repetitively added the velocity of the sphere repetively increased. As the velocities started to aproach 0.1254 m/sec the added weights had less and less effect on increasing the velocity. We conclude that as the velocity increased so did the drag force of the water. **

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RESPONSE -->

My exp. Vidoes aren't working for 1-14

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13:20:51

query univ phy problem 14.85 (14.89 10th edition) half-area constriction then open to outflow at dist h1 below reservoir level, tube from lower reservoir into constricted area, same fluid in both. Find ht h2 to which fluid in lower tube rises.

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RESPONSE -->

G-PHY

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13:20:58

** The fluid exits the narrowed part of the tube at atmospheric pressure. The widened part at the end of the tube is irrelevant--it won't be filled with fluid. So Bernoulli's Equation will tell you that the fluid velocity in this part is vExit such that .5 rho vExit^2 = rho g h1.

Now compare three points: point 1, in the narrowed tube; point 2 at the top of the fluid in the lower tube; and point 3 at the level of the fluid surface in the lower container.

At point 1 the pressure is atmospheric and velocity is vExit. Pressure is atmospheric because there is no pressure loss within the tube, since friction and viscosity are both assumed negligible.

At point 2 fluid velocity is zero and since there is no fluid between the narrowed tube and this point there is no net rho g h contribution to Bernoulli's equation. So we have .5 rho v1^2 + P1 = .5 rho v2^2 + P2. P1 is atmospheric and v1 is vExit from above, while v2 = 0 so P2 = atmospheric pressure + .5 rho vExit^2 = atmospheric pressure + rho g h1.

Now comparing point 2 with point 3 we see that there is a difference h in the fluid altitude, with velocity 0 at both points and atmospheric pressure at point 3. Thus P2 + rho g h2 = P3 + rho g h3, or (atmospheric pressure + rho g h1) + rho g h2 = atmospheric pressure + rho g h3. Thus rho g (h3 - h2) = rho g h1 and h3 - h2, which is the height of the fluid in the lower tube, is just equal to h1.

If we assume that somehow the fluid manages to expand on escaping the narrowed tube so that it fills the once-again-widened tube, and exits with vExit as above, then the velocity in the narrowed tube will be 2 * vExit. This leads to the conclusion that pressure change from small to large tube is .5 rho (2 vExit)^2 - .5 rho vExit^2 = .5 rho (3 vExit^2). Since pressure is atmospheric in the large tube, pressure in the small tube is atmospheric pressure + 3 ( .5 rho vExit^2). If we use this pressure for point 1 and follow the steps given above we conclude that h3 - h2, the height of the fluid column in the lower tube, is 3 h1. This is the book's answer. Again I don't have the problem in front of me and I might have missed something, but the idea of the fluid expanding to refill the larger pipe doesn't seem consistent with the behavior of even ideal liquids, which are pretty much incompressible at ordinary pressures. However note that I am sometimes wrong when I disagree with the textbook's solution. **

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RESPONSE -->

G-PHY

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13:21:07

query univ phy problem 14.85 (14.89 10th edition) half-area constriction then open to outflow at dist h1 below reservoir level, tube from lower reservoir into constricted area, same fluid in both. Find ht h2 to which fluid in lower tube rises.

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RESPONSE -->

G-PHY

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13:21:19

** The fluid exits the narrowed part of the tube at atmospheric pressure. The widened part at the end of the tube is irrelevant--it won't be filled with fluid. So Bernoulli's Equation will tell you that the fluid velocity in this part is vExit such that .5 rho vExit^2 = rho g h1.

Now compare three points: point 1, in the narrowed tube; point 2 at the top of the fluid in the lower tube; and point 3 at the level of the fluid surface in the lower container.

At point 1 the pressure is atmospheric and velocity is vExit. Pressure is atmospheric because there is no pressure loss within the tube, since friction and viscosity are both assumed negligible.

At point 2 fluid velocity is zero and since there is no fluid between the narrowed tube and this point there is no net rho g h contribution to Bernoulli's equation. So we have .5 rho v1^2 + P1 = .5 rho v2^2 + P2. P1 is atmospheric and v1 is vExit from above, while v2 = 0 so P2 = atmospheric pressure + .5 rho vExit^2 = atmospheric pressure + rho g h1.

Now comparing point 2 with point 3 we see that there is a difference h in the fluid altitude, with velocity 0 at both points and atmospheric pressure at point 3. Thus P2 + rho g h2 = P3 + rho g h3, or (atmospheric pressure + rho g h1) + rho g h2 = atmospheric pressure + rho g h3. Thus rho g (h3 - h2) = rho g h1 and h3 - h2, which is the height of the fluid in the lower tube, is just equal to h1.

If we assume that somehow the fluid manages to expand on escaping the narrowed tube so that it fills the once-again-widened tube, and exits with vExit as above, then the velocity in the narrowed tube will be 2 * vExit. This leads to the conclusion that pressure change from small to large tube is .5 rho (2 vExit)^2 - .5 rho vExit^2 = .5 rho (3 vExit^2). Since pressure is atmospheric in the large tube, pressure in the small tube is atmospheric pressure + 3 ( .5 rho vExit^2). If we use this pressure for point 1 and follow the steps given above we conclude that h3 - h2, the height of the fluid column in the lower tube, is 3 h1.

This is the book's answer. Again I don't have the problem in front of me and I might have missed something, but the idea of the fluid expanding to refill the larger pipe doesn't seem consistent with the behavior of liquids, which are pretty much incompressible at ordinary pressures. However note that I am sometimes wrong when I disagree with the textbook's solution. **

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RESPONSE -->

G-PHY

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Fy|tz{o߱ͳ∗G~

assignment #007

ىjؔަ|

Physics II

06-21-2006

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13:46:49

Query set 5 problems 16-20

explain how we calculate the average force exerted by a particle of mass m moving at speed v which collides at a time interval `dt elastically and at a right angle with a solid wall

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RESPONSE -->

The average force is equal to the average rate of momentum change. Which is equal to the momentum change divided by the 'dt. The momentum change is found by multiplying velocity by the mass of the particle.

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13:49:17

** The impulse exerted on a particle in a collision is the change in the momentum of that particle during a collision.

The impulse-momentum theorem says that the change in momentum in a collision is equal to the impulse, the average force * the time interval between collisions.

The average force is thus change in momentum / time interval; the time interval is the round-trip distance divided by the velocity, or 2L / v so the average force is -2 m v / ( 2L / v) = m v^2 / L

If there were N such particles the total average force would be N * m v^2 / L

If the directions are random we distribute the force equally over the 3 dimensions of space and for one direction we get get 1/3 the force found above, or 1/3 N * m v^2 / L.

This 3-way distribution of force is related to the fact that for the average velocity vector we have v^2 = vx^2 + vy^2 + vz^2, where v is average magnitude of velocity and vx, vy and vz the x, y and z components of the velocity (more specifically the rms averages--the square root of the average of the squared components). **

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RESPONSE -->

Ok I understand

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13:52:11

Summarize the relationship between the thermal energy that goes into the system during a cycle, the work done by the system during a cycle, and the thermal energy removed or dissipated during the cycle.

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RESPONSE -->

The thernal energy going into a system has to equal the work done by the system plus the thermal enegy dissipated by the system. The less thermal energy dissipated during the cycle the efficient the systme is

e=W/Qin

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13:52:20

** Work-energy is conserved within an isolated system. So the thermal energy that goes into the system must equal the total of the work done by the system and the thermal energy removed from the system. What goes in must come out, either in the form of work or thermal energy. **

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RESPONSE -->

Yes

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13:56:21

If you know the work done by a thermodynamic system during a cycle and the thermal energy removed or dissipated during the cycle, how would you calculate the efficiency of the cycle?

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RESPONSE -->

The efficiency of the system is the ratio of work done and thermal energy going into the system. The thermal energy going in is equal to Work +Qout. So if you add these two together and divide by the work done you'll have the efficiency of the system

e=W/Qin=W/(W+Qout)

or e= (Qin-Qout/Qin)

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13:56:34

** STUDENT SOLUTION: Efficiency is work done / energy input. Add the amount thermal energy removed to the amount of work done to get the input. Then, divide work by the energy input. **

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RESPONSE -->

Yes

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13:59:25

prin phy and gen phy problem 15.2, cylinder with light frictionless piston atm pressure, 1400 kcal added, volume increases slowly from 12.0 m^3 to 18.2 m^3. Find work and chagne in internal energy.

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RESPONSE -->

When 1400kcal of heat is added to gas in a piston at atm, the volume is observed to increase slowly from 12.0m^3 to 18.2m^3. Calculate (a) the work done by the gas, and (b) the change in internal energy of the gas.

Thus 'dV=6.2m^3 and Q=1400kcal(4.186x10^3)=5.86x10^6J

(a)W=P'dV= (1.013x10^3)(6.2m^3)=6.28x10^5J

(b)'dU=Q-W so 'dU=5.86x10^6J-6.28x10^5J=5.232x10^6J

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13:59:52

Work done at constant pressure is P `dV, so the work done in this situation is

`dW = P `dV = 1 atm * (18.2 m^3 - 12 m^3) = (101.3 * 10^3 N/m^2) * (6.2 m^3) = 630 * 10^3 N * m = 6.3 * 10^5 J.

A total of 1400 kcal = 1400 * 4200 J = 5.9 * 10^6 J of thermal energy is added to the system, the change in internal energy is

`dU = `dQ - `dW = 5.9*10^6 J - 6.3 * 10^5 J = 5.9 * 10^6 J - .63 * 10^6 J = 5.3 * 10^6 J.

It is worth thinking about the P vs. V graph of this process. The pressure P remains constant at 101.3 * 10^3 J as the volume changes from 12 m^3 to 18.2 m^3, so the graph will be a straight line segment from the point (12 m^3, 101.3 * 10^3 J) to the point (18.2 m^3, 101.3 * 10^3 J). This line segment is horizontaland the region above the horizontal axis and beneath the segment is a rectangle whose width is 6.2 * 10^3 m^3 and whose altitude is 101.3 * 10^3 N/m^2; its area is therefore the product of its altitude and width, which is 6.3 * 10^5 N m, or 6.3 * 10^5 J, the same as the word we calculated above.

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RESPONSE -->

Sounds good to me

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14:06:44

prin phy and gen phy problem 15.5, 1.0 L at 4.5 atm isothermally expanded until pressure is 1 atm then compressed at const pressure to init volume, final heated to return to original volume. Sketch and label graph.

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RESPONSE -->

The graph has the Pressure on the vertical (y) axis and the Volume on the horizonatal (x) axis. From top to bottom the pressure shows 4.5atm down to 1 atm and from left to right the volume changes form 1 to 4.5L.

There is a slope concave line from 4.5atm to 4.5L representing the Isothermal expansion, and a striaght line from 4.5L to 1L repesenting the Isobaric compression

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14:08:16

When a confined ideal gas is expanded isothermally its pressure and volume change, while the number of moled and the temperature remain constant. Since PV = n R T, it follows that P V remains constant.

In the initial state P = 4.5 atm and V = 1 liter, so P V = 4.5 atm * 1 liter = 4.5 atm * liter (this could be expressed in standard units since 1 atm = 101.3 kPa = 101.3 * 10^3 N/m^2 and 1 liters = .001 m^3, but it's more convenient to first sketch and label the graph in units of atm and liters). During the isothermal expansion, therefore, since P V remains constant we have

P V = 4.5 atm liters. At a pressure of 1 atm, therefore, the volume will be V = 4.5 atm liter / P = 4.5 atm liter / (1 atm) = 4.5 liters.

The graph follows a curved path from (1 liter, 4.5 atm) to (4.5 liters, 1 atm).

At the gas is compressed at constant pressure back to its initial 1 liter volume, the pressure remains constant so the graph follows a horizontal line from (4.5liters, 1 atm) to (1 liter, 1 atm). Note that this compression is accomplished by cooling the gas, or allowing it to cool.

Finally the gas is heated at constant volume until its pressure returns to 4.5 atm. The constant volume dictates that the graph follow a vertical line from (1 liter, 1 atm) back to (4.5 liters, 1 atm).

The graph could easily be relabeled to usestandard metric units.

1 atm = 101.3 kPa = 101.3 * 10^3 Pa = 101.3 * 10^3 N/m^2, so

4.5 atm = 4.5 * 101.3 * 10^3 Pa = 4.6 * 10^3 Pa = 4.6 * 10^3 N/m^2.

1 liter = .001 m^3 so 4.5 liters = 4.5 m^3.

Since P V = 4.5 atm liters, P = 4.5 atm liters / V. This is of the form P = c / V, with c a constant. For positive values of V, this curve descendsfrom a vertical asymptote with the vertical axis (the V axis) through the point (1, c) then approaches a horizontal asymptote with the horizontal axis. For c = 4.5 atm liters, the curve therefore passes through the point (1 liter, 4.5 atm). As we have seen it also passes through (4.5 liters, 1 atm).

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RESPONSE -->

I left out the portion for the IsoVolmetric change from 1atm to 4.5atm because the querry question did not ask for it, it was included in my HW that was turned in.

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14:13:49

gen phy problem 15.12, a-c curved path `dW = -35 J, `dQ = -63 J; a-b-c `dW = - 48 J

gen phy how much thermal energy goes into the system along path a-b-c and why?

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RESPONSE -->

a-c, W=-35J, Q=-63J

a-b-c, W=-48J

a)What is Q for path a-b-c? Qabc=(-48J)

b)If Pa=0.5Pb, what is W for c-d-a? W= 48J

c)What is Q for c-d-a? Q= 48J

d)What is Ua-Uc? 'dU=(-63J-(-35J))=-28J

e)If Ud-Uc=5J, what is Q for d-a? W=0, Q='dU =5J

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E|Đҗl}}

assignment #007

ىjؔަ|

Physics II

06-21-2006

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14:20:26

Query set 5 problems 16-20

explain how we calculate the average force exerted by a particle of mass m moving at speed v which collides at a time interval `dt elastically and at a right angle with a solid wall

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RESPONSE -->

I've already don the section as I was working thu this querry I clicked on diplay notes and it crashed. I'll pick up whrer I left off. I had just finished 15-12 text question

I'll delete the interim for you

OK we're back we it crashed.

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14:31:13

gen phy How are the work done by the system, the thermal energy added to the system and the change in the internal energy of the system related, and what is this relationship have to do with conservation of energy?

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RESPONSE -->

The thermal energy added to the system must equal the work performed and thethermal energy dissipated by the system.

conservation of energy states that the energy in must equal the energy out. Which the energy out is the Work plus the energy dissipated.

As for as the change in internal energy, if work is done by the system the internal energy is reduced if the work is done on the system the internal energy will increase.

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14:31:38

** If a system does work it tends to reduce internal energy, so `dW tends to decrease `dU. If thermal energy is added to the system `dQ tends to increase `dU. This leads to the conclusion that `dU = `dQ - `dW. Thus for example if `dW = -48 J and `dU = -28 J, `dQ = `dU + `dW = -28 J + -48 J = -76 J. **

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RESPONSE -->

This basically what I said

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14:36:54

gen phy How does the halving of pressure caused a halving of the magnitude of the work, and why is the work positive instead of negative as it was in the process a-b-c?

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RESPONSE -->

Well I'm not sure what a-b-c is referenced to but Work is equal to Force times distance or Pressure times 'dV,

Work will be positive is the work is performed on the system and negitive if its done by the system

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14:38:00

** Work is the area under the pressure vs. volume curve. If you have half the pressure between two volumes the graph has half the altitude, which leads to half the area.

The 'width' of a region is final volume - initial volume. If the direction of the process is such that final volume is less than initial volume (i.e., going 'backwards', in the negative x direction) then with 'width' is negative and the area is negative. **

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RESPONSE -->

OK I thought we were referring to the same curve but wasn't sure. Then expanding on what I said it makes sence

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14:38:35

.

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RESPONSE -->

I clicked Next question now I see nothing, I'll try again

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14:38:48

query univ phy problem 19.56 (17.40 10th edition) compressed air engine, input pressure 1.6 * 10^6 Pa, output 2.8 * 10^5 Pa, assume adiabatic.

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RESPONSE -->

G_PHY

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14:39:03

** For an adiabatic process in an ideal gas you know that PV = nRT and PV^`gamma is constant.

You are given P1 and P2, and you want T2 > 273 K to prevent formation of frost.

Assume T2 = P2 V2 / (n R) = 273 K and n R = (P2 V2) / 273 K .

Then T1 = P1 V1 / (n R) = P1 V1 * 273 K / (P2 V2) = (P1 / P2) * (V1 / V2) * 273 K.

Since PV^`gamma = constant it follows that V1 / V2 = (P2 / P1)^(1/`gamma) = (P1 / P2)^(-1/`gamma).

Thus T1 = (P1 / P2) ( P1 / P2)^(-1/`gamma) * 273 K = (P1 / P2)^(1 - 1/`gamma) = (P1 / P2)^(1-1/1.4) * 273 K = (P1 / P2)^.29 * 273 K = 5.6^.29 * 273 K = 443 K, approx. **

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G_PHY

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14:39:09

query univ 19.62 (17.46 10th edition) .25 mol oxygen 240 kPa 355 K. Isobaric to double vol, isothermal back, isochoric to original pressure.

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G_PHY

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14:39:18

** .25 mol oxygen at 240 kPa occupies about V = n R T / P = .25 mol * 8.31 J / (mol K) * 355 K / (2.4 * 10^5 N/m^2) = .003 m^3, very approximately.

Doubling volume, `dV = 2 * V - V = V = .003 m^2 and P = 2.4 * 10^5 Pa so P `dv = 700 J, very approximately.

During isothermal compression we have n = const and T = const so P = n R T / V. Compressing to half the volume, since PV = const, gets us to double the pressure, so max pressure is 2 * 240 kPA = 480 kPa.

To get work we integrate P dV. Integral of P dV is calculated from antiderivative n R T ln | V |; integrating between V1 and V2 we have n R T ln | V2 | - n R T ln | V1 | = n R T ln | V2 / V1 |. In this case V2 = V and V1 = 2 V so V2 / V1 = 1/2 and we have `dW = n R T ln(1/2) = .25 mol * 8.31 J/(mol K) * 710 K * (-.7) = -1000 J, approx.

So net work is about 700 J - 1000 J = -300 J **

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G_PHY

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14:39:24

univ phy describe your graph of P vs. V

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G_PHY

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14:39:29

** The graph proceeds horizontally to the right from original P and V to doubled V, then to the left along a curve that increases at an incr rate as we move to the left (equation P = 2 P0 V0 / V) until we're just above the starting point, then vertically down to the starting pt. **

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G_PHY

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14:39:35

univ phy What is the temperature during the isothermal compression?

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G_PHY

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14:39:40

** If vol doubles at const pressure then temp doubles to 710 K, from which isothermal compression commences. So the compression is at 710 K. **

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G_PHY

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14:39:45

univ phy What is the max pressure?

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G_PHY

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14:39:49

** It starts the isothermal at the original 240 kPa and its volume is halved at const temp. So the pressure doubles to 480 kPa. **

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G_PHY

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۟v爙؅

assignment #008

ىjؔަ|

Physics II

06-21-2006

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14:46:29

prin phy and gen phy problem 15.19 What is the maximum efficiency of a heat engine operating between temperatures of 380 C and 580 C?

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What is the maximum efficiency of a heat engine whose operating temperatures are 580*C(853K) and 380*C(653K)?

eideal =1-(TL/TH)=1-(653K/853K)=.2345=23.45%

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14:46:42

The maximum possible efficiency is (T_h - T_c) / T_h, where T_h and T_c are the absolute max and min operating temperatures.

T_h is (580 + 273)K = 853 K and T_c is (380 + 273) K = 653 K, so the maximum theoretical efficiency is

max efficiency = (T_h - T_c) / T_h = (853 K - 653 K) / (853 K) = .23, approx.

This means that the work done by this engine will be not greater than about 23% of the thermal energy that goes into it.

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Yes

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14:47:50

query gen phy problem 15.26 source 550 C -> Carnot eff. 28%; source temp for Carnot eff. 35%?

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A heat engine utilizes a heat source at 550*C and has an ideal (Carnot) efficiency of 28%. To increase the efficiency to 35% what must be the new temperature of the heat source?

eideal=1-(TL/TH)

.28=1-(TL/823K)

TL=(1-e)( TH)=592.6K

TH= TL /(1-.28) is held constant so the new TH

The new TH is TH= TL /(1-.35) and since is held constant

TH-New= TL/(1-.35)= 592.6K/(1-.35)=911.54K or 638.54*C

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14:48:08

** Carnot efficiency is eff = (Th - Tc) / Th.

Solving this for Tc we multiply both sides by Th to get

eff * Th = Th - Tc so that

Tc = Th - eff * Th = Th ( 1 - eff).

We note that all temperatures must be absolute so we need to work with the Kelvin scale (adding 273 C to the Celsius temperature to get the Kelvin temperature)

If Th = 550 C = 823 K and efficiency is 30% then we have

Tc =823 K * ( 1 - .28) = 592 K.

Now we want Carnot efficiency to be 35% for this Tc. We solve eff = (Th - Tc) / Th for Th:

Tc we multiply both sides by Th to get

eff * Th = Th - Tc so that

eff * Th - Th = -Tc and

Tc = Th - eff * Th or

Tc = Th ( 1 - eff) and

Th = Tc / (1 - eff).

If Tc = 576 K and eff = .35 we get

Th = 592 K / ( 1 - .35 ) = 592 C / .6 = 912 K, approx.

This is (912 - 273) C = 639 C. **

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Yes

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14:48:20

univ phy problem 20.44 (18.40 10th edition) ocean thermal energy conversion 6 C to 27 C

At 210 kW, what is the rate of extraction of thermal energy from the warm water and the rate of absorption by the cold water?

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G-PHY

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14:48:23

** work done / thermal energy required = .07 so thermal energy required = work done / .07.

Translating directly to power, thermal energy must be extracted at rate 210 kW / .07 = 30,000 kW. The cold water absorbs what's left after the 210 kW go into work, or 29,790 kW.

Each liter supplies 4186 J for every degree, or about 80 kJ for the 19 deg net temp change. Needing 30,000 kJ/sec this requires about 400 liters / sec, or well over a million liters / hour.

Comment from student: To be honest, I was suprised the efficiency was so low.

Efficiency is low but the energy is cheap and environmental impact in the deep ocean can be negligible so the process can be economical, if a bit ugly. **

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RESPONSE -->

G-PHY

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DOwѕ螳ͭ

assignment #009

ىjؔަ|

Physics II

06-21-2006

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14:54:25

Query introductory set 6, problems 1-10

explain how we know that the velocity of a periodic wave is equal to the product of its wavelength and frequency

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Since the frequency is how many peak-to-peak cycles of the travelling wave has past in a unit of time and the wave length is the distance between the peaks we can find the velocity, which is distance traveled in a unit of time, by multiplying frequency by the wavelength

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14:54:43

** we know how many wavelength segments will pass every second, and we know the length of each, so that multiplying the two gives us the velocity with which they must be passing **

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In a more general statement Yes

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14:54:48

** we know how many wavelength segments will pass every second, and we know the length of each, so that multiplying the two gives us the velocity with which they must be passing **

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14:58:45

explain how we can reason out that the period of a periodic wave is equal to its wavelength divided by its velocity

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The period, time required for one cylce of a periodic wave is the inverse of its frequency, the cycles per second.

So if v=f*Wavelength, and T=1/f, and f=velocity/wavelength

Then

T=wavelength/velocity

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14:58:59

** If we know how far it is between peaks (wavelength) and how fast the wavetrain is passing (velocity) we can divide the distance between peaks by the velocity to see how much time passes between peaks at a given point. That is, period is wavelength / velocity. **

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Yes

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15:16:34

explain why the equation of motion at a position x along a sinusoidal wave is A sin( `omega t - x / v) if the equation of motion at the x = 0 position is A sin(`omega t)

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The x/v is the time lag distance/velocity, and sonce distance is zero, x=0 (refernce point) the equation simplifies to

A sin(`omega t)

The time lag is the time required for the wave to propagate from x = 0 to some.

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15:17:12

** the key is the time delay. Time for the disturbance to get from x = 0 to position x is x / v. What happens at the new position is delayed by time x/v, so what happens there at clock time t happened at x=0 when clock time was t = x/v.

In more detail: If x is the distance down the wave then x / v is the time it takes the wave to travel that distance. What happens at time t at position x is what happened at time t - x/v at position x=0.

That expression should be y = sin(`omega * (t - x / v)).

}

The sine function goes from -1 to 0 to 1 to 0 to -1 to 0 to 1 to 0 ..., one cycle after another. In harmonic waves the motion of a point on the wave (think of the motion of a black mark on a white rope with vertical pulses traveling down the rope) will go thru this sort of motion (down, middle, up, middle, down, etc.) as repeated pulses pass.

If I'm creating the pulses at my end, and that black mark is some distance x down in rope, then what you see at the black mark is what I did at time x/v earlier. **

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RESPONSE -->

A lot more detailed but the same result

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15:26:59

Query introductory set six, problems 11-14

given the length of a string how do we determine the wavelengths of the first few harmonics?

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The wavelength is the time it would take for a wave to travel down the string and back, so the wavelength would be 2*L of the string.

'lambda=2L for its fundamental frequency.

Then for the first 3 harmonis, 2nd, 3rd and 4th harmonics we would have 2,3,4 half wavelengths.

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15:27:11

** As wavelength decreases you can fit more half-waves onto the string. You can fit one half-wave, or 2 half-waves, or 3, etc..

So you get

1 half-wavelength = string length, or wavelength = 2 * string length; using `lambda to stand for wavelength and L for string length this would be

1 * 1/2 `lambda = L so `lambda = 2 L.

For 2 wavelengths fit into the string you get

2 * 1/2 `lambda = L so `lambda = L.

For 3 wavelengths you get

3 * 1/2 `lambda = L so `lambda = 2/3 L; etc.

}

Your wavelengths are therefore 2L, L, 2/3 L, 1/2 L, etc.. **

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yes

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15:31:07

Given the wavelengths of the first few harmonics and the velocity of a wave disturbance in the string, how do we determine the frequencies of the first few harmonics?

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The harmonic frequencies are multiples of the fundemental frequency which is equal to the velocity divided by the wavelength. So you could find the funemental frequency and multiply it bey 2,3, and 4 for the 2nd, 3rd, and 4th harmonic frequency.

Or take the velocity and divide it by the wavelength for that harmonic and find the frequency

f=v/'lambda

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15:31:17

** The frequency is the number of crests passing per unit of time.

We can imagine a 1-second chunk of the wave divided into segments each equal to the wavelength. The number of peaks is equal to the length of the entire chunk divided by the length of a 1-wavelength segment. This is the number of peaks passing per second.

So frequency is equal to the wave velocity divided by the wavelength. **

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Yes sir

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15:34:48

Given the tension and mass density of a string how do we determine the velocity of the wave in the string?

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RESPONSE -->

The velocity of the string can be found by dividing the tension by the mass density and taking the square root of the result because

v='sqrt(Ft/(m/L))

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15:35:01

** We divide tension by mass per unit length and take the square root:

v = sqrt ( tension / (mass/length) ). **

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Yes

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15:40:50

gen phy explain in your own words the meaning of the principal of superposition

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Superposition is when two waves travelling in opposite direction meet and there displacements (amplitude and phase) are summed together to form a new wave at this point.

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15:41:05

** the principle of superposition tells us that when two different waveforms meet, or are present in a medium, the displacements of the two waveforms are added at each point to create the waveform that will be seen. **

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Says the same thing

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15:44:45

gen phy what does it mean to say that the angle of reflection is equal to the angle of incidence?

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It means that a when a wave hits something in its path the angle at which it struck the object will be the same as the angle of the reflected wave.

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15:44:53

** angle of incidence with a surface is the angle with the perpendicular to that surface; when a ray comes in at a given angle of incidence it reflects at an equal angle on the other side of that perpendicular **

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Yes

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{ᄞy˃M^R|

assignment #010

ىjؔަ|

Physics II

06-21-2006

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Your work on this assignment is very good. Let me know if you have questions.