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Basic Illustration Exercises in Hawking Radiation
(Notes II )
Roa, Ferdinand J. P.
Exercise A.4.4
(page 142 of [1])
Solutions to R(r) with vanishing 𝜔 and M
We take that both M and 𝜔 vanish and by a simple transformation 𝑟 → 𝑧
(15a)
𝑧 =
𝑟 − 𝐺𝑀𝑞
𝐺𝑀𝑞
= −
𝐺𝑀𝑞 − 𝑟
𝐺𝑀𝑞
We transform the given D.E. (12f) for R(r) into its Legendre form
(15b)
𝑑
𝑑𝑧
((1 − 𝑧2 )
𝑑𝑅
𝑑𝑧
) + 𝜇 𝜃
( 𝜇 𝜃 + 1) 𝑅 = 0
There are two regular singular points (RSP): 𝑧0 = −1, +1 that correspond to two values r = 0, 𝐺𝑀𝑞 ,
respectively.
First we may try the substitution
(15c)
𝑦 = 1 − 𝑧
to obtain
(15d)
𝑑
𝑑𝑦
( 𝑦(2 − 𝑦)
𝑑𝑅
𝑑𝑦
) + 𝜇 𝜃
( 𝜇 𝜃 + 1) 𝑅 = 0
and put the solution in power series form
(15e)
𝑅 = ∑ 𝑎 𝑛 𝑦 𝑠+𝑛
∞
𝑛=0
With this power series solution, we can immediately put (15d) into
(15f)
∑[ 𝜇 𝜃
( 𝜇 𝜃 + 1) − ( 𝑠 + 𝑛)( 𝑠 + 𝑛 + 1)] 𝑎 𝑛 𝑦 𝑆+𝑛
+ ∑ 2( 𝑠 + 𝑛)2
∞
𝑛=0
∞
𝑛=0
𝑎 𝑛 𝑦 𝑆+𝑛−1
= 0
Let us note that in (15d) we have an operator
(15g)
𝐿 ≡ 𝑦(2 − 𝑦)
𝑑2
𝑑𝑦2
+ 2(1 − 𝑦)
𝑑
𝑑𝑦
+ 𝜇 𝜃
( 𝜇 𝜃 + 1)
This operator as applied on (15e) yields, in the lowest power in y at 𝑛 = 0,
(15h)
𝐿[ 𝑅( 𝑦, 𝑠)] = 2𝑎0 𝑠2
𝑦 𝑠−1
and as the condition
(15i)
𝐿[ 𝑅( 𝑦, 𝑠)] = 0
is imposed for 𝑅( 𝑦, 𝑠) to be a solution, then we obtain the repeated values of 𝑠
(15j)
𝑠 = 0, 0
Let us also note that we have two commuting operators,
𝑑
𝑑𝑠
and 𝐿 so to have, in the lowest power in y at
𝑛 = 0,
(15k)
𝑑
𝑑𝑠
𝐿[ 𝑅( 𝑦, 𝑠)] = 𝐿 [
𝑑
𝑑𝑠
𝑅( 𝑦, 𝑠)] = 4𝑎0 𝑠 𝑦 𝑠−1
+ 2𝑎0 𝑠2
𝑦 𝑠−1
𝑙𝑛𝑦
where to follow as 𝑠 = 0
(15L)
𝑑
𝑑𝑠
𝐿[ 𝑅( 𝑦, 𝑠)] = 𝐿 [
𝑑
𝑑𝑠
𝑅( 𝑦, 𝑠)] = 0
Now, let us take 𝑠 = 0 and write one solution at this s-value in the form,
(16a)
𝑅1
( 𝑦, 𝑠 = 0) = 𝑅1
( 𝑦) = ∑ 𝑎 𝑛(0)𝑦 𝑛
∞
𝑛=0
and to choose( arbitrarily) 𝑎0
(0) = 1. The polynomial L(y) resulting from the operation 𝐿[ 𝑅1
( 𝑦, 𝑠 = 0)] is
obtained in the form
(16b)
𝐿( 𝑦) = ∑[ 𝜇 𝜃
( 𝜇 𝜃 + 1) − ( 𝑛 )( 𝑛 + 1 )] 𝑎 𝑛 𝑦 𝑆+𝑛
+ ∑ 2( 𝑛 )2
∞
𝑛=0
∞
𝑛=0
𝑎 𝑛(0)𝑦 𝑛−1
= 0
Note that we can make the shift 𝑛 → 𝑛 − 1. As 𝑅1
( 𝑦, 𝑠 = 0) must satisfy the condition 𝐿[ 𝑅1
( 𝑦, 𝑠 = 0)] =
0 and with the shift 𝑛 → 𝑛 − 1 in the first major term in L(y), we get the recurrence relation between
𝑎 𝑛(0) coefficients ( ∀𝑛 ≥ 1 ).
(16c)
𝑎 𝑛
(0) =
𝑛( 𝑛 − 1) − 𝜇 𝜃 (𝜇 𝜃 + 1)
2𝑛2
𝑎 𝑛−1
(0)
By repeated use of this recurrence relation we can write any coefficient 𝑎 𝑚(0) in terms of 𝑎0
(0) = 1
(16d)
𝑎 𝑚
(0) = −𝜇 𝜃
( 𝜇 𝜃 + 1)[(1)(2) − 𝜇 𝜃
( 𝜇 𝜃 + 1)] [(2)(3) − 𝜇 𝜃
( 𝜇 𝜃 + 1)]
×
[(3)(4) − 𝜇 𝜃
( 𝜇 𝜃 + 1)] ⋯ [( 𝑚 − 1) 𝑚 − 𝜇 𝜃
( 𝜇 𝜃 + 1)]
(2) 𝑚 (𝑚!)2
The series 𝑅1((1 − 𝑧), 𝑠 = 0) can terminate at the qth term as when 𝑎 𝑞 = 0, given ( 𝑞 − 1) 𝑞 =
𝜇 𝜃
( 𝜇 𝜃 + 1), where 𝑞 = 𝜇 𝜃 + 1. The recurrence formula (16c) shows that higher terms following the qth
term vanish also.
In crude form therefore, we write the Legendre polynomial for solution (16a) as
(16e)
𝑃𝜇 𝜃
= 𝑅1
𝜇 𝜃
((1 − 𝑧), 𝑠 = 0) = ∑ 𝑎 𝑛
𝜇 𝜃
(0)(1 − 𝑧) 𝑛
𝜇 𝜃
𝑛=0
𝑎0
𝜇 𝜃 (0) = 1, 𝑓𝑜𝑟 ∀𝜇 𝜃
For example, we have the first two of these polynomials:
(16f1)
𝑃1 = 𝑎0
1
+ 𝑎1
1 (1 − 𝑧) = 𝑧
𝑎1
1
(0) = −1
𝑎0
1
(0) = 1
𝑛𝑜𝑡𝑒𝑑: 𝑎2
1
(0) = 0
𝑃2 =
1
2
(3𝑧2
− 1)
𝑎0
2
(0) = 1
𝑎1
2 (0) = −3
𝑎2
2
(0) = 3
2⁄
Note: To be continued.
Ref’s
[1] Townsend, P. K., Blackholes – Lecture Notes, http://xxx.lanl.gov/abs/gr-qc/9707012
[2] Carroll, S. M., Lecture Notes On General Relativity, arXiv:gr-qc/9712019
[3] Gravitation and Spacetime, Ohanian, H. C., New York: W. W. Norton & Company Inc. copyright
1976
[4]Gravitation And Relativity, Bowler, M. G., Pergamon Press Inc., Maxwell House, Fairview
Park, ElmsFord, New York 1053, U. S. A., copyright 1976
[5] J. Foster, J. D. Nightingale, A SHORT COURSE IN GENERAL RELATIVITY, 2nd edition copyright
1995, Springer-Verlag, New York, Inc.,
[6]Arfken, G. B., Weber, H. J., Mathematical Methods For Physicists, Academic Press, Inc., U. K., 1995
[7]van Baal, P., A Course In Field Theory
[8]Siegel, W., Fields, http://insti.physics.sunysb.edu/~/siegel/plan.html
[9] Griffiths, D. J., Introduction To Elementary Particles, John Wiley & Sons, Inc., USA, 1987
[10]Rainville, E. D., Bedient, P. E., Elementary Differential Equations, Macmillan Publishing Co., Inc.,
New York, USA, 1981
[11]Pennisi, L., Elements of Complex Variables, 2nd edition, Holy, Rinehart & Winston, 1973
[12]Milton, A., Stegun, I., Handbook of Mathematical Functions, http://www.math.ucla.edu/~cbm/aands/,
http://th.physik.uni-frankfurt.de/~scherer/AbramovitzStegun/
Marion, J. B., Classical Dynamics of Particles and Systems, Academic Press Inc., New
York, 1965
Pennisi, L., Elements of Complex Variables, 2nd edition, Holy, Rinehart & Winston,
1973, pp. 223
http://www.math.ucla.edu/~cbm/aands/
http://th.physik.uni-frankfurt.de/~scherer/AbramovitzStegun/
E., Merzbacher, Quantum Mechanics, 2nd Edition, John Wiley & Sons, New York, 1970
[2] Pratt, S., Quantum Mechanics, Lecture Notes, http://www.nscl.msu.edu/~pratt/phy851
[3]Sakurai, J. J., Modern Quantum Mechanics, Addison-Wesley, 1994
[4]F. J. Dyson, ADVANCED QUANTUM MECHANICS, arXiv:quant-ph/0608140v1
Arfken, G. B., Weber, H. J., Mathematical Methods For Physicists, Academic Press, Inc., U. K., 1995

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Hawkinrad a source_notes ii _secured

  • 1. Basic Illustration Exercises in Hawking Radiation (Notes II ) Roa, Ferdinand J. P. Exercise A.4.4 (page 142 of [1]) Solutions to R(r) with vanishing 𝜔 and M We take that both M and 𝜔 vanish and by a simple transformation 𝑟 → 𝑧 (15a) 𝑧 = 𝑟 − 𝐺𝑀𝑞 𝐺𝑀𝑞 = − 𝐺𝑀𝑞 − 𝑟 𝐺𝑀𝑞 We transform the given D.E. (12f) for R(r) into its Legendre form (15b) 𝑑 𝑑𝑧 ((1 − 𝑧2 ) 𝑑𝑅 𝑑𝑧 ) + 𝜇 𝜃 ( 𝜇 𝜃 + 1) 𝑅 = 0 There are two regular singular points (RSP): 𝑧0 = −1, +1 that correspond to two values r = 0, 𝐺𝑀𝑞 , respectively. First we may try the substitution (15c) 𝑦 = 1 − 𝑧 to obtain (15d) 𝑑 𝑑𝑦 ( 𝑦(2 − 𝑦) 𝑑𝑅 𝑑𝑦 ) + 𝜇 𝜃 ( 𝜇 𝜃 + 1) 𝑅 = 0 and put the solution in power series form (15e) 𝑅 = ∑ 𝑎 𝑛 𝑦 𝑠+𝑛 ∞ 𝑛=0 With this power series solution, we can immediately put (15d) into (15f) ∑[ 𝜇 𝜃 ( 𝜇 𝜃 + 1) − ( 𝑠 + 𝑛)( 𝑠 + 𝑛 + 1)] 𝑎 𝑛 𝑦 𝑆+𝑛 + ∑ 2( 𝑠 + 𝑛)2 ∞ 𝑛=0 ∞ 𝑛=0 𝑎 𝑛 𝑦 𝑆+𝑛−1 = 0 Let us note that in (15d) we have an operator
  • 2. (15g) 𝐿 ≡ 𝑦(2 − 𝑦) 𝑑2 𝑑𝑦2 + 2(1 − 𝑦) 𝑑 𝑑𝑦 + 𝜇 𝜃 ( 𝜇 𝜃 + 1) This operator as applied on (15e) yields, in the lowest power in y at 𝑛 = 0, (15h) 𝐿[ 𝑅( 𝑦, 𝑠)] = 2𝑎0 𝑠2 𝑦 𝑠−1 and as the condition (15i) 𝐿[ 𝑅( 𝑦, 𝑠)] = 0 is imposed for 𝑅( 𝑦, 𝑠) to be a solution, then we obtain the repeated values of 𝑠 (15j) 𝑠 = 0, 0 Let us also note that we have two commuting operators, 𝑑 𝑑𝑠 and 𝐿 so to have, in the lowest power in y at 𝑛 = 0, (15k) 𝑑 𝑑𝑠 𝐿[ 𝑅( 𝑦, 𝑠)] = 𝐿 [ 𝑑 𝑑𝑠 𝑅( 𝑦, 𝑠)] = 4𝑎0 𝑠 𝑦 𝑠−1 + 2𝑎0 𝑠2 𝑦 𝑠−1 𝑙𝑛𝑦 where to follow as 𝑠 = 0 (15L) 𝑑 𝑑𝑠 𝐿[ 𝑅( 𝑦, 𝑠)] = 𝐿 [ 𝑑 𝑑𝑠 𝑅( 𝑦, 𝑠)] = 0 Now, let us take 𝑠 = 0 and write one solution at this s-value in the form, (16a) 𝑅1 ( 𝑦, 𝑠 = 0) = 𝑅1 ( 𝑦) = ∑ 𝑎 𝑛(0)𝑦 𝑛 ∞ 𝑛=0 and to choose( arbitrarily) 𝑎0 (0) = 1. The polynomial L(y) resulting from the operation 𝐿[ 𝑅1 ( 𝑦, 𝑠 = 0)] is obtained in the form (16b) 𝐿( 𝑦) = ∑[ 𝜇 𝜃 ( 𝜇 𝜃 + 1) − ( 𝑛 )( 𝑛 + 1 )] 𝑎 𝑛 𝑦 𝑆+𝑛 + ∑ 2( 𝑛 )2 ∞ 𝑛=0 ∞ 𝑛=0 𝑎 𝑛(0)𝑦 𝑛−1 = 0
  • 3. Note that we can make the shift 𝑛 → 𝑛 − 1. As 𝑅1 ( 𝑦, 𝑠 = 0) must satisfy the condition 𝐿[ 𝑅1 ( 𝑦, 𝑠 = 0)] = 0 and with the shift 𝑛 → 𝑛 − 1 in the first major term in L(y), we get the recurrence relation between 𝑎 𝑛(0) coefficients ( ∀𝑛 ≥ 1 ). (16c) 𝑎 𝑛 (0) = 𝑛( 𝑛 − 1) − 𝜇 𝜃 (𝜇 𝜃 + 1) 2𝑛2 𝑎 𝑛−1 (0) By repeated use of this recurrence relation we can write any coefficient 𝑎 𝑚(0) in terms of 𝑎0 (0) = 1 (16d) 𝑎 𝑚 (0) = −𝜇 𝜃 ( 𝜇 𝜃 + 1)[(1)(2) − 𝜇 𝜃 ( 𝜇 𝜃 + 1)] [(2)(3) − 𝜇 𝜃 ( 𝜇 𝜃 + 1)] × [(3)(4) − 𝜇 𝜃 ( 𝜇 𝜃 + 1)] ⋯ [( 𝑚 − 1) 𝑚 − 𝜇 𝜃 ( 𝜇 𝜃 + 1)] (2) 𝑚 (𝑚!)2 The series 𝑅1((1 − 𝑧), 𝑠 = 0) can terminate at the qth term as when 𝑎 𝑞 = 0, given ( 𝑞 − 1) 𝑞 = 𝜇 𝜃 ( 𝜇 𝜃 + 1), where 𝑞 = 𝜇 𝜃 + 1. The recurrence formula (16c) shows that higher terms following the qth term vanish also. In crude form therefore, we write the Legendre polynomial for solution (16a) as (16e) 𝑃𝜇 𝜃 = 𝑅1 𝜇 𝜃 ((1 − 𝑧), 𝑠 = 0) = ∑ 𝑎 𝑛 𝜇 𝜃 (0)(1 − 𝑧) 𝑛 𝜇 𝜃 𝑛=0 𝑎0 𝜇 𝜃 (0) = 1, 𝑓𝑜𝑟 ∀𝜇 𝜃 For example, we have the first two of these polynomials: (16f1) 𝑃1 = 𝑎0 1 + 𝑎1 1 (1 − 𝑧) = 𝑧 𝑎1 1 (0) = −1 𝑎0 1 (0) = 1 𝑛𝑜𝑡𝑒𝑑: 𝑎2 1 (0) = 0 𝑃2 = 1 2 (3𝑧2 − 1) 𝑎0 2 (0) = 1 𝑎1 2 (0) = −3 𝑎2 2 (0) = 3 2⁄
  • 4. Note: To be continued. Ref’s [1] Townsend, P. K., Blackholes – Lecture Notes, http://xxx.lanl.gov/abs/gr-qc/9707012 [2] Carroll, S. M., Lecture Notes On General Relativity, arXiv:gr-qc/9712019 [3] Gravitation and Spacetime, Ohanian, H. C., New York: W. W. Norton & Company Inc. copyright 1976 [4]Gravitation And Relativity, Bowler, M. G., Pergamon Press Inc., Maxwell House, Fairview Park, ElmsFord, New York 1053, U. S. A., copyright 1976 [5] J. Foster, J. D. Nightingale, A SHORT COURSE IN GENERAL RELATIVITY, 2nd edition copyright 1995, Springer-Verlag, New York, Inc., [6]Arfken, G. B., Weber, H. J., Mathematical Methods For Physicists, Academic Press, Inc., U. K., 1995 [7]van Baal, P., A Course In Field Theory [8]Siegel, W., Fields, http://insti.physics.sunysb.edu/~/siegel/plan.html [9] Griffiths, D. J., Introduction To Elementary Particles, John Wiley & Sons, Inc., USA, 1987 [10]Rainville, E. D., Bedient, P. E., Elementary Differential Equations, Macmillan Publishing Co., Inc., New York, USA, 1981 [11]Pennisi, L., Elements of Complex Variables, 2nd edition, Holy, Rinehart & Winston, 1973 [12]Milton, A., Stegun, I., Handbook of Mathematical Functions, http://www.math.ucla.edu/~cbm/aands/, http://th.physik.uni-frankfurt.de/~scherer/AbramovitzStegun/ Marion, J. B., Classical Dynamics of Particles and Systems, Academic Press Inc., New York, 1965 Pennisi, L., Elements of Complex Variables, 2nd edition, Holy, Rinehart & Winston, 1973, pp. 223 http://www.math.ucla.edu/~cbm/aands/ http://th.physik.uni-frankfurt.de/~scherer/AbramovitzStegun/
  • 5. E., Merzbacher, Quantum Mechanics, 2nd Edition, John Wiley & Sons, New York, 1970 [2] Pratt, S., Quantum Mechanics, Lecture Notes, http://www.nscl.msu.edu/~pratt/phy851 [3]Sakurai, J. J., Modern Quantum Mechanics, Addison-Wesley, 1994 [4]F. J. Dyson, ADVANCED QUANTUM MECHANICS, arXiv:quant-ph/0608140v1 Arfken, G. B., Weber, H. J., Mathematical Methods For Physicists, Academic Press, Inc., U. K., 1995