Export citation

Export citation

Choose format for download:

Download Citation
  • Access by Xinjiang University

Absorption of a massive scalar field by a charged black hole

Carolina L. Benone1,*, Ednilton S. de Oliveira1,†, Sam R. Dolan2,‡, and Luís C. B. Crispino1,§

  • 1Faculdade de Física, Universidade Federal do Pará, 66075-110 Belém, Pará, Brazil
  • 2Consortium for Fundamental Physics, School of Mathematics and Statistics, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, United Kingdom

  • *lben.carol@gmail.com
  • esdeoliveira@gmail.com
  • s.dolan@sheffield.ac.uk
  • §crispino@ufpa.br

Phys. Rev. D 89, 104053 – Published 27 May, 2014

DOI: https://doi.org/10.1103/PhysRevD.89.104053

Abstract

We calculate the absorption cross section of a massive neutral scalar field impinging upon a Reissner-Nordström black hole. First, we derive key approximations in the high- and low-frequency regimes. Next, we develop a numerical method to compute the cross section at intermediate frequencies, and present a selection of results. Finally, we draw together our complementary approaches to give a quantitative full-spectrum description of absorption.

See Also

Addendum to “Absorption of a massive scalar field by a charged black hole”

Carolina L. Benone, Ednilton S. de Oliveira, Sam R. Dolan, and Luís C. B. Crispino
Phys. Rev. D 95, 044035 (2017)

Article Text

References (37)

  1. J. M. Bardeen, B. Carter, and S. W. Hawking, Commun. Math. Phys. 31, 161 (1973).
  2. A. Celotti, J. C. Miller, and D. W. Sciama, Classical Quantum Gravity 16, A3 (1999).
  3. R. Narayan and J. E. McClintock, arXiv:1312.6698.
  4. A. M. Green, arXiv:1403.1198.
  5. S. Aretakis, Annales de l’Institut Henri Poincare, Section A: Physique Theorique 12, 1491 (2011).
  6. J. Lucietti, K. Murata, H. S. Reall, and N. Tanahashi, J. High Energy Phys. 03 (2013) 035.
  7. E. S. Oliveira, L. C. Crispino, and A. Higuchi, Phys. Rev. D 84, 084048 (2011).
  8. J. A. Futterman, F. A. Handler, and R. A. Matzner, Scattering From Black Holes (Cambridge University Press, Cambridge, England, 1988).
  9. G. Aad et al. (ATLAS Collaboration), Phys. Lett. B 716, 1 (2012).
  10. C. F. Macedo, P. Pani, V. Cardoso, and L. C. Crispino, Astrophys. J. 774, 48 (2013).
  11. W. Unruh, Phys. Rev. D 14, 3251 (1976).
  12. E. Jung and D. Park, Classical Quantum Gravity 21, 3717 (2004).
  13. C. Doran, A. Lasenby, S. Dolan, and I. Hinder, Phys. Rev. D 71, 124020 (2005).
  14. S. Dolan, C. Doran, and A. Lasenby, Phys. Rev. D 74, 064005 (2006).
  15. J. Castineiras, L. C. Crispino, and D. P. M. Filho, Phys. Rev. D 75, 024012 (2007).
  16. E. Jung, S. Kim, and D. Park, Phys. Lett. B 602, 105 (2004).
  17. Y. Decanini, A. Folacci, and M. O. E. Hadj, Phys. Rev. D 89, 084066 (2014).
  18. Y. Decanini, A. Folacci, and M. O. E. Hadj, arXiv:1401.0321.
  19. J. G. Rosa and S. R. Dolan, Phys. Rev. D 85, 044043 (2012).
  20. J. Barranco, A. Bernal, J. C. Degollado, A. Diez-Tejedor, M. Megevand, M. Alcubierre, D. Núñez, and O. Sarbach, Phys. Rev. Lett. 109, 081102 (2012).
  21. J. Barranco, A. Bernal, J. C. Degollado, A. Diez-Tejedor, M. Megevand, M. Alcubierre, D. Núñez, and O. Sarbach, Phys. Rev. D 89, 083006 (2014).
  22. R. Brito, V. Cardoso, and P. Pani, Phys. Rev. D 88, 064006 (2013).
  23. H. Okawa, H. Witek, and V. Cardoso, arXiv:1401.1548.
  24. P. Pani, V. Cardoso, L. Gualtieri, E. Berti, and A. Ishibashi, Phys. Rev. Lett. 109, 131102 (2012).
  25. S. R. Dolan, Phys. Rev. D 87, 124026 (2013).
  26. H. Yoshino and H. Kodama, arXiv:1312.2326.
  27. L. C. Crispino and E. S. Oliveira, Phys. Rev. D 78, 024011 (2008).
  28. N. Sanchez, Phys. Rev. D 18, 1030 (1978).
  29. Y. Décanini, G. Esposito-Farèse, and A. Folacci, Phys. Rev. D 83, 044032 (2011)
  30. Y. Décanini, A. Folacci, and B. Raffaelli, Classical Quantum Gravity 28, 175021 (2011).
  31. Y. Décanini, A. Folacci, and B. Raffaelli, Phys. Rev. D 84, 084035 (2011).
  32. S. R. Dolan and A. C. Ottewill, Classical Quantum Gravity 26, 225003 (2009).
  33. In Ref. [11] it is shown that the low-frequency limit of the transmission coefficient for small black holes behaves as ω2l+2, so that the l=0 contribution is dominant in this limit.

  34. M. Abramowitz and I. A. Stegun, Handbook of Mathematical Functions with Formulas, Graphics and Mathematical Tables (Dover Publications, New York, 1965), 9th ed.
  35. L. C. Crispino, S. R. Dolan, and E. S. Oliveira, Phys. Rev. D 79, 064022 (2009).
  36. Z. Li and C. Bambi, J. Cosmol. Astropart. Phys. 01 (2014) 041.
  37. C. F. B. Macedo, L. C. S. Leite, E. S. Oliveira, S. R. Dolan, and L. C. B. Crispino, Phys. Rev. D 88, 064033 (2013).

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation