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Use the result of Problem 2.42 to calculate the temperature of a black hole, in terms of its mass M. (The energy is Mc2. ) Evaluate the resulting expression for a one-solar-mass black hole. Also sketch the entropy as a function of energy, and discuss the implications of the shape of the graph.

Short Answer

Expert verified

The required expression is T=hc3162GMc2kand for one-solar-mass of a black hole, the temperature can be calculated be 6.1510-8K.

The graph below depicts the entropy as a function of energy which is a concave up graph.

Step by step solution

01

Given

The expression for the entropy of a black hole is given as:

S=82GM2hck..........(1)

Where,

Gis the gravitational constant, Mis mass, his Planck's constant, cis the speed of light, and kis the Boltzmann's constant

The energy of the black hole is given by Einstein's relation as:

U=Mc2..........(2)

02

Calculation for Temperature

Mathematically, temperature can be defined as:

1T=SU..........(3)

Where,

Sis the change in entropy and Uis the change in the internal energy of the body.

Equation (1) can be modified as:

role="math" localid="1646995322714" S=82GM2hckc4c4S=82G(Mc2)2hc5k

By replacing Mc2as U, we get,

role="math" localid="1646997428892" S=82GU2hc5k..........(4)

Now, by substituting this value of Sin equation (3), we get,

1T=SU=U82GU2hc5k1T=162GUhc5kT=hc5162GUk

By resusbstituting the value of Uin the above equation, we get the desired result in terms of mass,

T=hc3162GMc2k

For a solar mass black hole, M=21030kg.

Also, by substituting 6.6710-11m3kg-1s-2for G, 6.6210-34J.sfor h, 1.3810-23J/Kfor kand 3108ms-1for cin the above equation, we get,

T=6.6210-34310831626.6710-11210301.3810-23T=6.1510-8K

03

Graph of entropy as a function of energy

Consider the equation (4),

S=82GU2hc5k

Here,

G,K,h,care all constants

Hence, it can be modified as:

SU2

Therefore, the graph of entropy as a function of energy can be sketched as follows:

It can be observed that the graph is a concave up graph. Objects exhibiting such behavior would have a negative heat capacity.

04

Final answer

The required expression is T=hc3162GMc2kand the temperature can be calculated to be 6.1510-8K. Also the graph of entropy as a function of energy which is a concave up graph, can be sketched as follows:

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Most popular questions from this chapter

Starting with the result of Problem 3.5, calculate the heat capacity of an Einstein solid in the low-temperature limit. Sketch the predicted heat capacity as a function of temperature.

Consider a monatomic ideal gas that lives at a height z above sea level, so each molecule has potential energy mgzin addition to its kinetic energy.

(a) Show that the chemical potential is the same as if the gas were at sea level, plus an additional term mgz:

(z)=-kTlnVN2mkTh23/2+mgz.

(You can derive this result from either the definition =-T(S/N)U,Vor the formula =(U/N)S,V.

(b) Suppose you have two chunks of helium gas, one at sea level and one at height z, each having the same temperature and volume. Assuming that they are in diffusive equilibrium, show that the number of molecules in the higher chunk is

N(z)=N(0)e-mgz/kT

in agreement with the result of Problem 1.16.

Consider an Einstein solid for which both N and q are much greater than 1. Think of each oscillator as a separate "particle."

(a) Show that the chemical potential is

role="math" localid="1646995468663" =-kTlnN+qN

(b) Discuss this result in the limits Nqand Nq, concentrating on the question of how much Sincreases when another particle carrying no energy is added to the system. Does the formula make intuitive sense?

Use the definition of temperature to prove the zeroth law of thermodynamics, which says that if system A is in thermal equilibrium with system B, and system B is in thermal equilibrium with system C, then system A is in thermal equilibrium with system C. (If this exercise seems totally pointless to you, you're in good company: Everyone considered this "law" to be completely obvious until 1931, when Ralph Fowler pointed out that it was an unstated assumption of classical thermodynamics.)

A liter of air, initially at room temperature and atmospheric pressure, is heated at constant pressure until it doubles in volume. Calculate the increase in its entropy during this process.

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