In this problem we will deal with simple thermodynamics model of a black hole. Assume that the properties of a black hole depend only on the mass of the black hole. (a) One characteristic of a black hole is the area of its event horizon. Roughly speaking, the event horizon is the boundary of the black hole. Inside this boundary, the gravity is so strong that even light cannot emerge from the region enclosed by the boundary. We shall write A = G°c®m°. Use dimensional analysis to find a, ß , and y. (b) One quantities in thermodynamics is entropy (S), that measure the disorder of a system. The relationship between entropy S, energy E and temperature 0 of a system is given as follow: = . For black holes, Bekenstein propose that the entropy is proportional the area of the black hole's event horizon S = nA, where n depends on c, k, G and h. Using dimensional analysis determine 7. (c) With the previous results, determine the temperature of the black hole, as a function of the mass. The energy of a black hole is E = mc². (d) The Stefan Boltzmann constant o is a can be written as k, = ah"®G*k{. Take a dimensionless constant a as one. Determine a, B, y and 8. (e) Assuming black hole is perfect blackbody , determine the rate of blackhole evapo- ration . dm (f) Determine how long for a black hole to evaporate completely if the initial mass is М.
In this problem we will deal with simple thermodynamics model of a black hole. Assume that the properties of a black hole depend only on the mass of the black hole. (a) One characteristic of a black hole is the area of its event horizon. Roughly speaking, the event horizon is the boundary of the black hole. Inside this boundary, the gravity is so strong that even light cannot emerge from the region enclosed by the boundary. We shall write A = G°c®m°. Use dimensional analysis to find a, ß , and y. (b) One quantities in thermodynamics is entropy (S), that measure the disorder of a system. The relationship between entropy S, energy E and temperature 0 of a system is given as follow: = . For black holes, Bekenstein propose that the entropy is proportional the area of the black hole's event horizon S = nA, where n depends on c, k, G and h. Using dimensional analysis determine 7. (c) With the previous results, determine the temperature of the black hole, as a function of the mass. The energy of a black hole is E = mc². (d) The Stefan Boltzmann constant o is a can be written as k, = ah"®G*k{. Take a dimensionless constant a as one. Determine a, B, y and 8. (e) Assuming black hole is perfect blackbody , determine the rate of blackhole evapo- ration . dm (f) Determine how long for a black hole to evaporate completely if the initial mass is М.
Modern Physics
3rd Edition
ISBN:9781111794378
Author:Raymond A. Serway, Clement J. Moses, Curt A. Moyer
Publisher:Raymond A. Serway, Clement J. Moses, Curt A. Moyer
Chapter2: Relativity Ii
Section: Chapter Questions
Problem 27P
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![In this problem we will deal with simple thermodynamics model of a black hole. Assume
that the properties of a black hole depend only on the mass of the black hole.
(a) One characteristic of a black hole is the area of its event horizon. Roughly speaking,
the event horizon is the boundary of the black hole. Inside this boundary, the gravity
is so strong that even light cannot emerge from the region enclosed by the boundary.
We shall write A = G°c®m°. Use dimensional analysis to find a, ß , and y.
(b) One quantities in thermodynamics is entropy (S), that measure the disorder of a
system. The relationship between entropy S, energy E and temperature 0 of a
system is given as follow: = . For black holes, Bekenstein propose that the
entropy is proportional the area of the black hole's event horizon S = nA, where n
depends on c, k, G and h. Using dimensional analysis determine 7.
(c) With the previous results, determine the temperature of the black hole, as a function
of the mass. The energy of a black hole is E = mc².
(d) The Stefan Boltzmann constant o is a can be written as k, = ah"®G*k{. Take a
dimensionless constant a as one. Determine a, B, y and 8.
(e) Assuming black hole is perfect blackbody , determine the rate of blackhole evapo-
ration .
dm
(f) Determine how long for a black hole to evaporate completely if the initial mass is
М.](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2Fa52b29af-a1a6-4f61-a3be-ceb9e559158c%2F1e46eea0-af8e-4fad-994b-5577f5c48e28%2Fa9loswa_processed.png&w=3840&q=75)
Transcribed Image Text:In this problem we will deal with simple thermodynamics model of a black hole. Assume
that the properties of a black hole depend only on the mass of the black hole.
(a) One characteristic of a black hole is the area of its event horizon. Roughly speaking,
the event horizon is the boundary of the black hole. Inside this boundary, the gravity
is so strong that even light cannot emerge from the region enclosed by the boundary.
We shall write A = G°c®m°. Use dimensional analysis to find a, ß , and y.
(b) One quantities in thermodynamics is entropy (S), that measure the disorder of a
system. The relationship between entropy S, energy E and temperature 0 of a
system is given as follow: = . For black holes, Bekenstein propose that the
entropy is proportional the area of the black hole's event horizon S = nA, where n
depends on c, k, G and h. Using dimensional analysis determine 7.
(c) With the previous results, determine the temperature of the black hole, as a function
of the mass. The energy of a black hole is E = mc².
(d) The Stefan Boltzmann constant o is a can be written as k, = ah"®G*k{. Take a
dimensionless constant a as one. Determine a, B, y and 8.
(e) Assuming black hole is perfect blackbody , determine the rate of blackhole evapo-
ration .
dm
(f) Determine how long for a black hole to evaporate completely if the initial mass is
М.
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