- Physical Review Journals
All JournalsPhysics Magazine

Physical Review D

Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Open Access

Impact of a dark boson mediated feeble interaction between dark matter and hadronic matter on the f-mode oscillation of neutron stars

Debashree Sen1,* and Atanu Guha2,†

  • *Contact author: debashreesen88@gmail.com
  • †Contact author: atanu@cnu.ac.kr
PDF

Phys. Rev. D 110, 103013 – Published 12 November, 2024

DOI: https://doi.org/10.1103/PhysRevD.110.103013

Abstract

We studied the possible presence of dark matter (DM) in neutron stars (NSs) and the structural properties of the DM admixed NSs (DMANSs) in one of our recent works [1]. The feeble interaction between the fermionic DM (χ) with the hadronic matter is introduced through a dark scalar (ϕ) and a dark vector (ξ) boson as mediators. The allowed range of the mass of the fermionic DM (mχ), for a particular range of DM Fermi momentum (kFχ), was obtained in the same work [1] with respect to the various astrophysical constraints on the structural properties of compact stars viz., the mass, radius, and tidal deformability. The present work is dedicated to the calculation and study of nonradial oscillation of the DMANSs using Cowling approximation. We particularly investigate the effect of the presence of DM on the fundamental (f) mode oscillation frequencies of the DMANSs utilizing the previously obtained range of mχ for four different hadronic models. In this work we thoroughly investigate how the individual and combined effects of mχ and kFχ affect the f-mode oscillation frequency. Within the framework of our DMANS models, for a particular value of kFχ, the range of fmaxDMANS, with respect to the allowed range of mχ, is also obtained in the present work for four different hadronic models. Since in the present era, the 1.4 and 2.01M⊙ NSs are of special interest after the detection of GW170817 and PSR J0740+6620, we particularly investigate, for the four hadronic models, the range of f1.4DMANS and f2.01DMANS with respect to the acceptable range of mχ corresponding to the range of kFχ.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (111)

  1. A. Guha and D. Sen, Phys. Rev. D 109, 043038 (2024).
  2. P. A. R. Ade et al. (Planck Collaboration), Astron. Astrophys. 594, A13 (2016).
  3. G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405, 279 (2005).
  4. N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A6 (2020).
  5. J. B. Bauer, D. J. E. Marsh, R. Hložek, H. Padmanabhan, and A. Laguë, Mon. Not. R. Astron. Soc. 500, 3162 (2020).
  6. M. Lisanti, in New Frontiers in Fields and Strings (World Scientific, Singapore, 2017), pp. 399–446.
  7. S. Profumo, in Searching for New Physics at Small and Large Scales (World Scientific, Singapore, 2013), pp. 143–189.
  8. R. Agnese et al. (SuperCDMS Collaboration), Phys. Rev. Lett. 121, 051301 (2018); 122, 069901(E) (2019).
  9. E. Aprile et al. (XENON Collaboration), Phys. Rev. Lett. 129, 161805 (2022).
  10. Q. Wang et al. (PandaX-II Collaboration), Chin. Phys. C 44, 125001 (2020).
  11. P. Agnes et al. (DarkSide Collaboration), Phys. Rev. Lett. 121, 111303 (2018).
  12. M. Crisler, R. Essig, J. Estrada, G. Fernandez, J. Tiffenberg, M. Sofo haro, T. Volansky, and T.-T. Yu (SENSEI Collaboration), Phys. Rev. Lett. 121, 061803 (2018).
  13. J. Aalbers et al. (LZ Collaboration), Phys. Rev. Lett. 131, 041002 (2023).
  14. W. B. Atwood et al. (Fermi-LAT Collaboration), Astrophys. J. 697, 1071 (2009).
  15. M. G. Aartsen et al. (IceCube Collaboration), Phys. Rev. Lett. 113, 101101 (2014).
  16. O. Adriani et al. (PAMELA Collaboration), Nature (London) 458, 607 (2009).
  17. O. Adriani et al. (PAMELA Collaboration), Phys. Rev. Lett. 111, 081102 (2013).
  18. L. Accardo et al. (AMS Collaboration), Phys. Rev. Lett. 113, 121101 (2014).
  19. M. Boudaud, J. Lavalle, and P. Salati, Phys. Rev. Lett. 119, 021103 (2017).
  20. O. Adriani et al. (CALET Collaboration), Phys. Rev. Lett. 119, 181101 (2017).
  21. O. Adriani et al., Phys. Rev. Lett. 120, 261102 (2018).
  22. M. Baryakhtar, J. Bramante, S. W. Li, T. Linden, and N. Raj, Phys. Rev. Lett. 119, 131801 (2017).
  23. A. Joglekar, N. Raj, P. Tanedo, and H.-B. Yu, Phys. Lett. B 809, 135767 (2020).
  24. N. F. Bell, G. Busoni, and S. Robles, J. Cosmol. Astropart. Phys. 06 (2019) 054.
  25. A. Joglekar, N. Raj, P. Tanedo, and H.-B. Yu, Phys. Rev. D 102, 123002 (2020).
  26. J. Bramante and N. Raj, Phys. Rep. 1052, 1 (2024).
  27. W. Husain, T. F. Motta, and A. W. Thomas, J. Cosmol. Astropart. Phys. 10 (2022) 028.
  28. W. Husain and A. W. Thomas, J. Phys. G 50, 015202 (2023).
  29. W. Husain, D. Sengupta, and A. W. Thomas, Universe 9, 307 (2023).
  30. D. Zhou, Universe 9, 484 (2023).
  31. A. Nelson, S. Reddy, and D. Zhou, J. Cosmol. Astropart. Phys. 07 (2019) 012.
  32. N. F. Bell, G. Busoni, S. Robles, and M. Virgato, J. Cosmol. Astropart. Phys. 03 (2021) 086.
  33. G. Panotopoulos and I. Lopes, Phys. Rev. D 96, 083004 (2017).
  34. A. Guha and D. Sen, J. Cosmol. Astropart. Phys. 09 (2021) 027.
  35. D. Sen and A. Guha, Mon. Not. R. Astron. Soc. 504, 3354 (2021).
  36. S. Shakeri and D. R. Karkevandi, Phys. Rev. D 109, 043029 (2024).
  37. D. R. Karkevandi, S. Shakeri, V. Sagun, and O. Ivanytskyi, Phys. Rev. D 105, 023001 (2022).
  38. C. H. Lenzi, M. Dutra, O. Lourenço, L. L. Lopes, and D. P. Menezes, Eur. Phys. J. C 83, 266 (2023).
  39. O. Lourenço, C. H. Lenzi, T. Frederico, and M. Dutra, Phys. Rev. D 106, 043010 (2022).
  40. I. Lopes and G. Panotopoulos, Phys. Rev. D 97, 024030 (2018).
  41. J. Ellis, G. Hütsi, K. Kannike, L. Marzola, M. Raidal, and V. Vaskonen, Phys. Rev. D 97, 123007 (2018).
  42. A. Li, F. Huang, and R.-X. Xu, Astropart. Phys. 37, 70 (2012).
  43. L. Tolos and J. Schaffner-Bielich, Phys. Rev. D 92, 123002 (2015).
  44. M. Deliyergiyev, A. Del Popolo, L. Tolos, M. Le Delliou, X. Lee, and F. Burgio, Phys. Rev. D 99, 063015 (2019).
  45. S. Mukhopadhyay, D. Atta, K. Imam, D. N. Basu, and C. Samanta, Eur. Phys. J. C 77, 440 (2017); 77, 553(E) (2017).
  46. J. C. Jiménez and E. S. Fraga, Universe 8, 34 (2022).
  47. G. Panotopoulos and I. Lopes, Phys. Rev. D 98, 083001 (2018).
  48. K.-L. Leung, M.-c. Chu, and L.-M. Lin, Phys. Rev. D 105, 123010 (2022).
  49. O. Lourenço, T. Frederico, and M. Dutra, Phys. Rev. D 105, 023008 (2022).
  50. T. Gleason, B. Brown, and B. Kain, Phys. Rev. D 105, 023010 (2022).
  51. Y. Dengler, J. Schaffner-Bielich, and L. Tolos, Phys. Rev. D 105, 043013 (2022).
  52. G. Panotopoulos and I. Lopes, Int. J. Mod. Phys. D 27, 1850093 (2018).
  53. Z. Miao, Y. Zhu, A. Li, and F. Huang, Astrophys. J. 936, 69 (2022).
  54. N. Rutherford, G. Raaijmakers, C. Prescod-Weinstein, and A. Watts, Phys. Rev. D 107, 103051 (2023).
  55. B. Bertoni, A. E. Nelson, and S. Reddy, Phys. Rev. D 88, 123505 (2013).
  56. S. A. Bhat and A. Paul, Eur. Phys. J. C 80, 544 (2020).
  57. M. Dutra, C. H. Lenzi, and O. Lourenço, Mon. Not. R. Astron. Soc. 517, 4265 (2022).
  58. B. Hong, Z. Ren, C. Wu, and X. Mu, Classical Quantum Gravity 40, 125007 (2023).
  59. X. Mu, B. Hong, X. Zhou, and Z. Feng, Astrophys. Space Sci. 368, 67 (2023).
  60. H. Zheng and L.-W. Chen, Astrophys. J. 831, 127 (2016).
  61. E. Fonseca et al., Astrophys. J. Lett. 915, L12 (2021).
  62. M. C. Miller et al., Astrophys. J. Lett. 918, L28 (2021).
  63. T. E. Riley et al., Astrophys. J. Lett. 918, L27 (2021).
  64. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Phys. Rev. Lett. 121, 161101 (2018).
  65. T. E. Riley et al., Astrophys. J. Lett. 887, L21 (2019).
  66. M. C. Miller et al., Astrophys. J. Lett. 887, L24 (2019).
  67. K. D. Kokkotas and B. G. Schmidt, Living Rev. Relativity 2, 2 (1999).
  68. N. Andersson and K. D. Kokkotas, Mon. Not. R. Astron. Soc. 299, 1059 (1998).
  69. H. K. Lau, P. T. Leung, and L. M. Lin, Astrophys. J. 714, 1234 (2010).
  70. T. K. Chan, Y. H. Sham, P. T. Leung, and L. M. Lin, Phys. Rev. D 90, 124023 (2014).
  71. H. Sotani and B. Kumar, Phys. Rev. D 104, 123002 (2021).
  72. T. Zhao and J. M. Lattimer, Phys. Rev. D 106, 123002 (2022).
  73. C. Vásquez Flores, Z. B. Hall, II, and P. Jaikumar, Phys. Rev. C 96, 065803 (2017).
  74. B. K. Pradhan and D. Chatterjee, Phys. Rev. C 103, 035810 (2021).
  75. A. Kunjipurayil, T. Zhao, B. Kumar, B. K. Agrawal, and M. Prakash, Phys. Rev. D 106, 063005 (2022).
  76. K. S. Thorne and A. Campolattaro, Astrophys. J. 149, 591 (1967).
  77. L. Lindblom and S. L. Detweiler, Astrophys. J. Suppl. Ser. 53, 73 (1983).
  78. T. G. Cowling, Mon. Not. R. Astron. Soc. 101, 367 (1941).
  79. H. Sotani, N. Yasutake, T. Maruyama, and T. Tatsumi, Phys. Rev. D 83, 024014 (2011).
  80. C. V. Flores and G. Lugones, Classical Quantum Gravity 31, 155002 (2014).
  81. N. Andersson and P. Pnigouras, Mon. Not. R. Astron. Soc. 489, 4043 (2019).
  82. A. Kumar, P. Thakur, and M. Sinha, Mon. Not. R. Astron. Soc. 530, 501 (2024).
  83. I. F. Ranea-Sandoval, O. M. Guilera, M. Mariani, and M. G. Orsaria, J. Cosmol. Astropart. Phys. 12 (2018) 031.
  84. C. Vásquez Flores, A. Parisi, C.-S. Chen, and G. Lugones, J. Cosmol. Astropart. Phys. 06 (2019) 051.
  85. B. K. Pradhan, D. Chatterjee, M. Lanoye, and P. Jaikumar, Phys. Rev. C 106, 015805 (2022).
  86. O. P. Jyothilakshmi, L. J. Naik, and V. Sreekanth, Eur. Phys. J. C 84, 427 (2024).
  87. H. C. Das, A. Kumar, S. K. Biswal, and S. K. Patra, Phys. Rev. D 104, 123006 (2021).
  88. H.-M. Liu, J.-B. Wei, Z.-H. Li, G. F. Burgio, H. C. Das, and H. J. Schulze, Phys. Rev. D 110, 023024 (2024).
  89. G. A. Lalazissis, J. Konig, and P. Ring, Phys. Rev. C 55, 540 (1997).
  90. N. K. Glendenning and S. A. Moszkowski, Phys. Rev. Lett. 67, 2414 (1991).
  91. S. Typel, G. Ropke, T. Klahn, D. Blaschke, and H. H. Wolter, Phys. Rev. C 81, 015803 (2010).
  92. G. A. Lalazissis, T. Niksic, D. Vretenar, and P. Ring, Phys. Rev. C 71, 024312 (2005).
  93. B.-N. Lu, E.-G. Zhao, and S.-G. Zhou, Phys. Rev. C 84, 014328 (2011).
  94. C.-J. Xia, T. Maruyama, A. Li, B. Y. Sun, W.-H. Long, and Y.-X. Zhang, Commun. Theor. Phys. 74, 095303 (2022).
  95. S. Tulin, H.-B. Yu, and K. M. Zurek, Phys. Rev. D 87, 115007 (2013).
  96. D. Sen and A. Guha, Mon. Not. R. Astron. Soc. 517, 518 (2022).
  97. S. W. Randall, M. Markevitch, D. Clowe, A. H. Gonzalez, and M. Bradac, Astrophys. J. 679, 1173 (2008).
  98. M. Bradac, D. Clowe, A. H. Gonzalez, P. Marshall, W. Forman, C. Jones, M. Markevitch, S. Randall, T. Schrabback, and D. Zaritsky, Astrophys. J. 652, 937 (2006).
  99. S. Tulin and H.-B. Yu, Phys. Rep. 730, 1 (2018).
  100. T. Hambye and L. Vanderheyden, J. Cosmol. Astropart. Phys. 05 (2020) 001.
  101. G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun. 185, 960 (2014).
  102. P. Gondolo and G. Gelmini, Nucl. Phys. B360, 145 (1991).
  103. A. Guha, P. S. B. Dev, and P. K. Das, J. Cosmol. Astropart. Phys. 02 (2019) 032.
  104. A. Das, T. Malik, and A. C. Nayak, Phys. Rev. D 99, 043016 (2019).
  105. A. G. Abac, C. C. Bernido, and J. P. H. Esguerra, Phys. Dark Universe 40, 101185 (2023).
  106. R. C. Tolman, Phys. Rev. 55, 364 (1939).
  107. J. R. Oppenheimer and G. M. Volkoff, Phys. Rev. 55, 374 (1939).
  108. T. Hinderer, Astrophys. J. 677, 1216 (2008).
  109. T. Hinderer, B. D. Lackey, R. N. Lang, and J. S. Read, Phys. Rev. D 81, 123016 (2010).
  110. Z.-Y. Zheng, T.-T. Sun, H. Chen, J.-B. Wei, G. F. Burgio, and H. J. Schulze, Phys. Rev. D 107, 103048 (2023).
  111. V. B. Thapa, M. V. Beznogov, A. R. Raduta, and P. Thakur, Phys. Rev. D 107, 103054 (2023).

Outline

Information

Phys. Rev. D 110, 103013– Published 12 November, 2024
  • Received 21 June 2024
  • Accepted 1 October 2024
Crossmark - Check for updates button
Creative Commons Logo

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation