|
|
Scattering and absorption of particles by a black hole involving a global monopole |
Shao Jian Zhou(邵建舟) and Wang Yong Jiu(王永久)† |
Institute of Physics, Hunan Normal University, Changsha 410081, China |
|
|
Abstract Under the conditions that the wavelength of a particle is much larger than its radius of central mass, and the Schwarzschild field is weak, the scattering of a particle has been studied by many researchers. They obtained that scalar and vector particles abide by Rutherforďs angle distribution by using the low level perturbation method and the scattered fielďs approximation in a weak field. The scattering cross section of a photon coincides with the section in Newton's field of point mass. We can obtain the photon's polarization effect by calculating the second-order perturbation in the linear Schwarzschild field. This article discusses the scattering and absorption of a particle by a black hole involving a global monopole by using the aforesaid method.
|
Received: 29 July 2011
Revised: 27 September 2011
Accepted manuscript online:
|
|
Fund: Project supported by the State Key Development Program for Basic Research of China(Grant No.2010CB832800),the Na-tional Natural Science Foundation of China(Grant No.10873004),the Scientific Research Fund of Hunan Provincial EducationDepartment,China(Grant No.08B051),and the Scientific Research Fund of Hunan Normal University |
Corresponding Authors:
Wang Yong-Jiu, E-mail:wyj@hunnu.edu.cn
E-mail: wyj@hunnu.edu.cn
|
Cite this article:
Shao Jian Zhou(邵建舟) and Wang Yong Jiu(王永久) Scattering and absorption of particles by a black hole involving a global monopole 2012 Chin. Phys. B 21 040404
|
[1] |
Matzner R A and Math J 1968 Phys. Rev. D 9 163
|
[2] |
Fabbri R 1975 Phys. Rev. D 12 933
|
[3] |
Peters P C 1976 Phys. Rev. D 13 775
|
[4] |
de Logi W K and Kovacs S J 1977 Phys. Rev. D 16 237
|
[5] |
Sanchez N G and Math J 1976 Phys. Rev. D 17 688
|
[6] |
Sanchez N G 1977 Phys. Rev. D 16 937
|
[7] |
Sanchez N G 1978 Phys. Rev. D 18 1030
|
[8] |
Sanchez N G 1978 Phys. Rev. D 18 1798
|
[9] |
Zhang T R and DeWitt-Morette C 1984 Phys. Rev. Lett. 18 2313
|
[10] |
Matzner R A, DeWitt-Morette C, Nelson B and Zhang T R 1985 Phys. Rev. D 31 1869
|
[11] |
Anninos P, DeWitt-Morette C, Matzner R A, Yioutas P and Zhang T R 1992 Phys. Rev. D 18 4477
|
[12] |
Andersson N 1995 Phys. Rev. D 52 1808
|
[13] |
Andersson N and Jensen B P 2001 arXiv. gr-qc/0011025
|
[14] |
Doran C J L and Lasenby A N 2002 Phys. Rev. D 52 024006
|
[15] |
Chen J H and Wang Y J 2011 Phys. Rev. D 20 030401
|
[16] |
Chen J H and Wang Y J 2011 Phys. Rev. D 55 813816
|
[17] |
Chandrasekhar S 1983 The Mathematical Theory of Black Holes (New York: Oxford University Press)
|
[18] |
Futterman J A H, Handler F A and Matzner R A 1988 Scattering from Black Hole (Cambridge: Cambridge University Press)
|
[19] |
Wang Y J 2008 Classic Black Hole and Quantum Black Hole (Beijing: Science Press)
|
No Suggested Reading articles found! |
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
Cited |
|
|
|
|
Altmetric
|
blogs
Facebook pages
Wikipedia page
Google+ users
|
Online attention
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
View more on Altmetrics
|
|
|