This problem investigates what fraction of the available charge must be transferred from one conductor to another to produce a typical contact potential. (a) As a rough approximation treat the conductors as10cmx 10 cm square plates2cm apart-a parallel-plate capacitors so thatq=CV , where C=σ0(0.01m2/0.02m). How much charge must be transferred from one plate to the other to produce a potential difference of 2V?(b) Approximately what fraction would this be of the total number of conduction electrons in a 100gpiece of copper. which has one conduction electron per atom?

Short Answer

Expert verified

The total charge required to produce 2Vthe across the capacitor isQ=9×1012C

The ratio of the two sets of electrons isR=6×1017

Step by step solution

01

Total chargeQ  on the plates of a capacitor and number of electrons N that would give rise to the total charge Q.

The equation for the total charge Qon the plates of a capacitor given a potentialV:

Q=CV

……. (1)

HereCis the capacitance of a (10cm)(10cm)parallel-plate capacitor (with a plate separation of 2cm), given by:

C=ε0(0.01m20.02m) …… (2)

The number of electronsNthat would give rise to the total chargeQwould be written as:

N=Qe

With e being the elementary unit charge on the electron. So then the 8.85×1012Cis used for theQ and 1.6×1019C for e:

N=Qe=(8.85×1012C)1.6×1019C=5.53×107

So that's the number of electrons needed to give rise to the2V

And0 is the permittivity of free space.

The atomic mass for copper of 63.546. Convert them to standard units:

(63.546u)(1.66×1027kg1u)=1.055×1025kg

02

Find the total charge involved to produce a potential of2 V .

(a)

Potential difference across capacitor=2V

To find the total charge involved to produce a potential of2V , equation (2) is inserted in forC in equation (1) , withε0 being 8.85×1012C2/N.m2and Vbeing2V , withε0 being 8.85×1012C2/N.m2and Vbeing2V :

Q=CV=ε0(0.01m20.02m)(V)=(8.85×1012C2Nm2)(0.01m20.02m)(2V)=8.85×1012C

03

Step 3:The ratio of two sets of electrons. 

(b)

Next, since there is one conduction electron per copper atom, the number of the electrons in the 100gsample can be found by just giving a look how many copper atoms it takes to make up the 100g. it can be expressed with the equation:

n=mamu

With being the number of electrons or atoms, the mass of the sample, and being the atomic mass of the copper atom. So then0.1kg is inserted in for the (since standard units are needed), and1.055*1025

kgfor the amu:

n=mamu=(0.1kg)(1.055×1025kg)=9.48×1023

So, there are9.48×1023 atoms/conduction electrons in the100g sample.

So then just divide the two of them to get the ratio:

R=Nn=(5.53×107)(9.48×1023)=5.83×1017

The ratio of the two sets of electrons isR=6×1017

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Figure 9.8 cannot do justice to values at the very highspeed end of the plot. This exercise investigates how small it really gets. However, although integrating the Maxwell speed distribution over the full range of speeds from 0 to infinity can be carried out (the so-called Gaussian integrals of Appendix K), over any restricted range, it is one of those integrals that. unfortunately. cannot be done in closed form. Using a computational aid of your choice. show that the fraction of molecules moving faster thanis; faster than6vrmsis-10-23; and faster than10vmsis~10-64. wherevrms" from Exercise 41, is3kBT/m. (Exercise 48 uses these values in an interesting application.)

A particle subject to a planet's gravitational pull has a total mechanical energy given by Emechanical=12mv2-GMmr, whereis the particle's mass.M the planet's mass, and Gthe gravitational constant6.67×10-11N·m3/kg2. It may escape if its energy is zero that is, if its positive KE is equal in magnitude to the negative PE holding if to the surface. Suppose the particle is a gas molecule in an atmosphere.

(a) Temperatures in Earth's atmosphere may reach 1000K. Referring to the values obtained in Exercise 45 and given that REarth=6.37×106mand MEarth=5.98×1024kg. should Earth be able to "hold on" to hydrogen (1g/mol)? 10 nitrogens (28g/mol)? (Note: An upper limit on the number of molecules in Earth's atmosphere is about 10-18).

(b) The moon's mass is 0.0123times Earth's. its radius 0.26 times Earth's, and its surface temperatures rise to 370K. Should it be able to hold on to these gases?

Verify that the probabilities shown in Table 9.1 for four distinguishable oscillators sharing energy 2δEagree with the exact probabilities given by equation (9-9).

What is special about a metastable Stale, and why is it so useful ina laser? Why wouldn't a non-metastable state at the same energy work?

Example 9.2 obtains a ratio of the number of particles expected in the n = 2state lo that in the ground state. Rather than the n = 2state, consider arbitrary n.

(a) Show that the ratio is numberofenergyEnnumberofenergyE1=n2e-13.6cV(1-n-2)/kBT

Note that hydrogen atom energies are En=-13.6eV/st2.

(b) What is the limit of this ratio as n becomes very large? Can it exceed 1? If so, under what condition(s)?

(c) In Example 9.2. we found that even at the temperature of the Sun's surface(~6000K), the ratio for n = 2 is only 10-8 . For what value of nwould the ratio be 0.01?

(d) Is it realistic that the number of atoms with high n could be greater than the number with low n ?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free