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Thebulk modulus of a substance is the ratio of a small decrease in pressure to the resulting fractional increase in volume:

B=-VdPdV.

Show thatB=(5/3)P, in the free electron gas model, and use your result in Problem 5.16(d) to estimate the bulk modulus of copper. Comment: The observed value is 13.4×1010N/m2, but don’t expect perfect agreement—after all, we’re neglecting all electron–nucleus and electron–electron forces! Actually, it is rather surprising that this calculation comes as close as it does.

Short Answer

Expert verified

B=53(3.84×1010N/m2)=6.4×1010N/m2

Step by step solution

01

Definition of bulk modulus of a substance

The volumetric stress to volumetric strain ratio for any given material is known as the bulk modulus.

02

Showing that B = (5/3) P in the free electron gas model

We need to find bulk modulus in the free electron gas model. And after that, we need to estimate the bulk modulus of copper from the previous problem.

p=2Etot3V=232kF55mρ5/3

P=(3π2)2/325mρ5/3=AV-5/3,A=2(3π2)2/3(Nq)5/35m.

Bulk modulus is equal to:

role="math" localid="1658144523557" B=-VdPdV=-V-53AV-8/3=53AV-5/3=53PB=53P

Degeneracy pressure of copper was P=3.84×1010Pa. So Bulk modulus, according to the formula is,For copper,

B=533.84×1010N/m2=6.4×1010N/m2.

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Most popular questions from this chapter

(a)Use Equation5.113 to determine the energy density in the wavelength rangedλ. Hint: setρ(ω)=ρ-(λ), and solve forρ(λ)-

(b)Derive the Wien displacement law for the wavelength at which the blackbody energy density is a maximum
λmax=2.90×10-3mKT

You'll need to solve the transcendental equation(5×x)=5e-x, using a calculator (or a computer); get the numerical answer accurate to three significant digits.

The ground state of dysprosium (element 66, in the 6th row of the Periodic Table)

is listed as Is5. What are the total spin, total orbital, and grand total angular

momentum quantum numbers? Suggest a likely electron configuration for

dysprosium.

Derive the Stefan-Boltzmann formula for the total energy density in blackbody radiation

EV=(π2kB415ħ3C3)T4=7.57×10-16Jm-3K-4T4

In view ofProblem 5.1, we can correct for the motion of the nucleus in hydrogen by simply replacing the electron mass with the reduced mass.

(a) Find (to two significant digits) the percent error in the binding energy of hydrogen (Equation 4.77) introduced by our use of m instead of μ.

E1=-m2h2e24π'2=-13.6eV(4.77).

(b) Find the separation in wavelength between the red Balmer lines n=3n=2for hydrogen and deuterium (whose nucleus contains a neutron as well as the proton).

(c) Find the binding energy of positronium (in which the proton is replaced by a positron—positrons have the same mass as electrons, but opposite charge).

(d) Suppose you wanted to confirm the existence of muonic hydrogen, in which the electron is replaced by a muon (same charge, but 206.77 times heavier). Where (i.e. at what wavelength) would you look for the “Lyman-α” line n=2n=1?.

a) Hund’s first rule says that, consistent with the Pauli principle, the state with the highest total spin (S) will have the lowest energy. What would this predict in the case of the excited states of helium?

(b) Hund’s second rule says that, for a given spin, the state with the highest total orbital angular momentum (L) , consistent with overall antisymmetrization, will have the lowest energy. Why doesn’t carbon haveL=2? Note that the “top of the ladder”(ML=L)is symmetric.

(c) Hund’s third rule says that if a subshell(n,l)is no more than half filled,
then the lowest energy level hasJ=lL-SI; if it is more than half filled, thenJ=L+Shas the lowest energy. Use this to resolve the boron ambiguity inProblem 5.12(b).

(d) Use Hund’s rules, together with the fact that a symmetric spin state must go with an antisymmetric position state (and vice versa) to resolve the carbon and nitrogen ambiguities in Problem 5.12(b). Hint: Always go to the “top of the ladder” to figure out the symmetry of a state.

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