Papers
Topics
Authors
Recent
Search
2000 character limit reached

Massive Scalar Field Perturbations of Black Holes Immersed in Chaplygin-Like Dark Fluid

Published 17 Mar 2024 in gr-qc and hep-th | (2403.11306v3)

Abstract: We consider massive scalar field perturbations in the background of black holes immersed in Chaplygin-like dark fluid (CDF), and we analyze the photon sphere modes, the de Sitter modes as well as the near extremal modes and discuss their dominance, by using the pseudospectral Chebyshev method and the third order Wentzel-Kramers-Brillouin approximation. We also discuss the impact of the parameter representing the intensity of the CDF on the families of quasinormal modes. Mainly, we find that the propagation of a massive scalar field is stable in this background, and it is characterized by quasinormal frequencies with a smaller oscillation frequency and a longer decay time compared to the propagation of the same massive scalar field within the Schwarzschild-de Sitter background.

Definition Search Book Streamline Icon: https://streamlinehq.com
References (49)
  1. U. Alam, V. Sahni, T. D. Saini and A. A. Starobinsky, “Is there supernova evidence for dark energy metamorphosis ?,” Mon. Not. Roy. Astron. Soc. 354, 275 (2004) [arXiv:astro-ph/0311364 [astro-ph]].
  2. R. R. Caldwell, “A Phantom menace?,” Phys. Lett. B 545, 23-29 (2002) [arXiv:astro-ph/9908168 [astro-ph]].
  3. R. R. Caldwell, M. Kamionkowski and N. N. Weinberg, “Phantom energy and cosmic doomsday,” Phys. Rev. Lett. 91, 071301 (2003) [arXiv:astro-ph/0302506 [astro-ph]].
  4. Á. O. F. de Almeida, L. Amendola and V. Niro, “Galaxy rotation curves in modified gravity models,” JCAP 08, 012 (2018) [arXiv:1805.11067 [astro-ph.GA]].
  5. J. Harada, “Cotton gravity and 84 galaxy rotation curves,” Phys. Rev. D 106, no.6, 064044 (2022) [arXiv:2209.04055 [gr-qc]].
  6. H. Shabani and P. H. R. S. Moraes, “Galaxy rotation curves in the f(R, T) gravity formalism,” Phys. Scripta 98, no.6, 065302 (2023) [arXiv:2206.14920 [gr-qc]].
  7. A. Y. Kamenshchik, U. Moschella and V. Pasquier, “An Alternative to quintessence,” Phys. Lett. B 511, 265-268 (2001) [arXiv:gr-qc/0103004 [gr-qc]].
  8. N. Bilic, G. B. Tupper and R. D. Viollier, “Unification of dark matter and dark energy: The Inhomogeneous Chaplygin gas,” Phys. Lett. B 535, 17-21 (2002) [arXiv:astro-ph/0111325 [astro-ph]].
  9. M. C. Bento, O. Bertolami and A. A. Sen, “Generalized Chaplygin gas, accelerated expansion and dark energy matter unification,” Phys. Rev. D 66, 043507 (2002) [arXiv:gr-qc/0202064 [gr-qc]].
  10. R. Sengupta, P. Paul, B. C. Paul and M. Kalam, “Can extended Chaplygin gas source a Hubble tension resolved emergent universe ?,” [arXiv:2307.02602 [gr-qc]].
  11. A. Abdullah, A. A. El-Zant and A. Ellithi, “Growth of fluctuations in Chaplygin gas cosmologies: A nonlinear Jeans scale for unified dark matter,” Phys. Rev. D 106, no.8, 083524 (2022) [arXiv:2108.03260 [astro-ph.CO]].
  12. X. Q. Li, B. Chen and L. l. Xing, “Charged Lovelock black holes in the presence of dark fluid with a nonlinear equation of state,” Eur. Phys. J. Plus 135, no.2, 175 (2020) [arXiv:1905.08156 [gr-qc]].
  13. F. Ferrer, A. Medeiros da Rosa, and C. M. Will, “ Dark matter spikes in the vicinity of kerr black holes,” Phys.Rev. D 96, 083014 (2017).
  14. S. Nampalliwar, S. Kumar, K. Jusufi, Q. Wu, M. Jamil, and P. Salucci, “Modeling the sgr a* black hole immersed in a dark matter spike,” The Astrophysical Journal 916,116 (2021).
  15. Z. Xu, J. Wang, and M. Tang, “Deformed black hole immersed in dark matter spike,” Journal of Cosmology and Astroparticle Physics 2021 (09), 007.
  16. K. Jusufi, M. Jamil, and T. Zhu, “Shadows of black hole surrounded by superfluid dark matter halo,“ The European Physical Journal C 80, 354 (2020).
  17. X. Hou, Z. Xu and J. Wang, “Rotating Black Hole Shadow in Perfect Fluid Dark Matter,” JCAP 12 (2018), 040 [arXiv:1810.06381 [gr-qc]].
  18. S. Haroon, M. Jamil, K. Jusufi, K. Lin and R. B. Mann, “Shadow and Deflection Angle of Rotating Black Holes in Perfect Fluid Dark Matter with a Cosmological Constant,” Phys. Rev. D 99 (2019) no.4, 044015 [arXiv:1810.04103 [gr-qc]].
  19. X. Hou, Z. Xu, M. Zhou and J. Wang, “Black hole shadow of Sgr A*{}^{*}start_FLOATSUPERSCRIPT * end_FLOATSUPERSCRIPT in dark matter halo,” JCAP 07 (2018), 015 [arXiv:1804.08110 [gr-qc]].
  20. K. Jusufi, “Black holes surrounded by Einstein clusters as models of dark matter fluid,” Eur. Phys. J. C 83, no.2, 103 (2023) [arXiv:2202.00010 [gr-qc]].
  21. R. A. Konoplya and A. Zhidenko, “Solutions of the Einstein Equations for a Black Hole Surrounded by a Galactic Halo,” Astrophys. J. 933, no.2, 166 (2022) [arXiv:2202.02205 [gr-qc]].
  22. E. Figueiredo, A. Maselli and V. Cardoso, “Black holes surrounded by generic dark matter profiles: Appearance and gravitational-wave emission,” Phys. Rev. D 107, no.10, 104033 (2023) [arXiv:2303.08183 [gr-qc]].
  23. S. V. M. C. B. Xavier, H. C. D. Lima, Junior. and L. C. B. Crispino, “Shadows of black holes with dark matter halo,” Phys. Rev. D 107, no.6, 064040 (2023) [arXiv:2303.17666 [gr-qc]].
  24. X. Q. Li, H. P. Yan, X. J. Yue, S. W. Zhou and Q. Xu, “Geodesic structure, shadow and optical appearance of black hole immersed in Chaplygin-like dark fluid,” [arXiv:2401.18066 [gr-qc]].
  25. A. Aragón, P. A. González, E. Papantonopoulos and Y. Vásquez, “Anomalous decay rate of quasinormal modes in Schwarzschild-dS and Schwarzschild-AdS black holes,” JHEP 08 (2020), 120 [arXiv:2004.09386 [gr-qc]].
  26. A. Aragón, P. A. González, E. Papantonopoulos and Y. Vásquez, “Quasinormal modes and their anomalous behavior for black holes in f⁢(R)𝑓𝑅f(R)italic_f ( italic_R ) gravity,” Eur. Phys. J. C 81 (2021) no.5, 407 [arXiv:2005.11179 [gr-qc]].
  27. R. D. B. Fontana, P. A. González, E. Papantonopoulos and Y. Vásquez, “Anomalous decay rate of quasinormal modes in Reissner-Nordström black holes,” Phys. Rev. D 103 (2021) no.6, 064005 [arXiv:2011.10620 [gr-qc]].
  28. R. Bécar, P. A. González, F. Moncada and Y. Vásquez, “Massive scalar field perturbations in Weyl black holes,” Eur. Phys. J. C 83, no.10, 942 (2023) [arXiv:2304.00663 [gr-qc]].
  29. R. A. Konoplya and A. V. Zhidenko, “Decay of massive scalar field in a Schwarzschild background,” Phys. Lett. B 609 (2005), 377-384 [arXiv:gr-qc/0411059 [gr-qc]].
  30. R. A. Konoplya and A. Zhidenko, “Stability and quasinormal modes of the massive scalar field around Kerr black holes,” Phys. Rev. D 73 (2006), 124040 [arXiv:gr-qc/0605013 [gr-qc]].
  31. S. R. Dolan, “Instability of the massive Klein-Gordon field on the Kerr spacetime,” Phys. Rev. D 76 (2007), 084001 [arXiv:0705.2880 [gr-qc]].
  32. O. J. Tattersall and P. G. Ferreira, “Quasinormal modes of black holes in Horndeski gravity,” Phys. Rev. D 97 (2018) no.10, 104047 [arXiv:1804.08950 [gr-qc]].
  33. M. Lagos, P. G. Ferreira and O. J. Tattersall, “Anomalous decay rate of quasinormal modes,” Phys. Rev. D 101 (2020) no.8, 084018 [arXiv:2002.01897 [gr-qc]].
  34. P. A. González, E. Papantonopoulos, J. Saavedra and Y. Vásquez, “Quasinormal modes for massive charged scalar fields in Reissner-Nordström dS black holes: anomalous decay rate,” JHEP 06 (2022), 150 [arXiv:2204.01570 [gr-qc]].
  35. R. Bécar, P. A. González and Y. Vásquez, “Quasinormal modes of a charged scalar field in Ernst black holes,” Eur. Phys. J. C 83, no.1, 75 (2023) [arXiv:2211.02931 [gr-qc]].
  36. A. Aragón, R. Bécar, P. A. González and Y. Vásquez, “Massive Dirac quasinormal modes in Schwarzschild–de Sitter black holes: Anomalous decay rate and fine structure,” Phys. Rev. D 103, no.6, 064006 (2021) [arXiv:2009.09436 [gr-qc]].
  37. K. Destounis, R. D. B. Fontana and F. C. Mena, “Accelerating black holes: quasinormal modes and late-time tails,” Phys. Rev. D 102, no.4, 044005 (2020) [arXiv:2005.03028 [gr-qc]].
  38. P. A. González, E. Papantonopoulos, Á. Rincón and Y. Vásquez, “Quasinormal modes of massive scalar fields in four-dimensional wormholes: Anomalous decay rate,” Phys. Rev. D 106 (2022) no.2, 024050 [arXiv:2205.06079 [gr-qc]].
  39. S. Alfaro, P. A. González, D. Olmos, E. Papantonopoulos and Y. Vásquez, “Quasinormal modes and bound states of massive scalar fields in generalized Bronnikov-Ellis wormholes,” [arXiv:2402.15575 [gr-qc]].
  40. G. Raposo, P. Pani, M. Bezares, C. Palenzuela and V. Cardoso, “Anisotropic stars as ultracompact objects in General Relativity,” Phys. Rev. D 99 (2019) no.10, 104072 [arXiv:1811.07917 [gr-qc]].
  41. B. Mashhoon, “Quasi-normal modes of a black hole,” Third Marcel Grossmann Meeting on General Relativity 1983.
  42. B. F. Schutz and C. M. Will, “Black Hole NormalL Modes: A Semianalytic Approach,” Astrophys. J. Lett. 291 (1985), L33-L36
  43. S. Iyer and C. M. Will, “Black Hole Normal Modes: A WKB Approach. 1. Foundations and Application of a Higher Order WKB Analysis of Potential Barrier Scattering,” Phys. Rev. D 35 (1987), 3621
  44. R. A. Konoplya, “Quasinormal behavior of the d-dimensional Schwarzschild black hole and higher order WKB approach,” Phys. Rev. D 68 (2003), 024018 [arXiv:gr-qc/0303052 [gr-qc]].
  45. J. Matyjasek and M. Opala, “Quasinormal modes of black holes. The improved semianalytic approach,” Phys. Rev. D 96 (2017) no.2, 024011 [arXiv:1704.00361 [gr-qc]].
  46. R. A. Konoplya, A. Zhidenko and A. F. Zinhailo, “Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations,” Class. Quant. Grav. 36 (2019), 155002 [arXiv:1904.10333 [gr-qc]].
  47. R. A. Konoplya and A. Zhidenko, “Quasinormal modes of black holes: From astrophysics to string theory,” Rev. Mod. Phys.  83, 793 (2011) [arXiv:1102.4014 [gr-qc]].
  48. Y. Hatsuda, “Quasinormal modes of black holes and Borel summation,” Phys. Rev. D 101, no.2, 024008 (2020) [arXiv:1906.07232 [gr-qc]].
  49. D. P. Du, B. Wang and R. K. Su, “Quasinormal modes in pure de Sitter space-times,” Phys. Rev. D 70, 064024 (2004) [arXiv:hep-th/0404047 [hep-th]].
Citations (2)
View on Semantic Scholar

Summary

No one has generated a summary of this paper yet.

Ai Sparkles Streamline Icon: https://streamlinehq.com Sign Up to Summarize

Paper to Video (Beta)

Whiteboard

No one has generated a whiteboard explanation for this paper yet.

Ai Sparkles Streamline Icon: https://streamlinehq.com Sign Up to Generate

Open Problems

We haven't generated a list of open problems mentioned in this paper yet.

Ai Sparkles Streamline Icon: https://streamlinehq.com Generate Now

Continue Learning

We haven't generated follow-up questions for this paper yet.

Ai Sparkles Streamline Icon: https://streamlinehq.com Generate Now

Collections

Sign up for free to add this paper to one or more collections.

User Circle Single Streamline Icon: https://streamlinehq.com Sign Up

Tweets

Sign up for free to view the 2 tweets with 4 likes about this paper.

User Circle Single Streamline Icon: https://streamlinehq.com Sign Up for Free