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Influence of dark matter on magnetized neutron stars

Vishal Parmar1,*, H. C. Das2,†, M. K. Sharma1, and S. K. Patra3,4

  • 1School of Physics and Materials Science, Thapar Institute of Engineering and Technology, Patiala 147004, India
  • 2INFN Sezione di Catania, Dipartimento di Fisica, Via S. Sofia 64, 95123 Catania, Italy
  • 3Institute of Physics, Sachivalaya Marg, Bhubaneswar 751005, India
  • 4Homi Bhabha National Institute, Training School Complex, Anushakti Nagar, Mumbai 400094, India

  • *physics.vishal01@gmail.com
  • †harish.d@iopb.res.in
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Phys. Rev. D 108, 083003 – Published 2 October, 2023

DOI: https://doi.org/10.1103/PhysRevD.108.083003

Abstract

Over the past two decades, significant strides have been made in the study of dark matter (DM) admixed neutron stars and their associated properties. However, an intriguing facet regarding the effect of DM on magnetized neutron stars still remains unexplored. This study is carried out to analyze the properties of DM admixed magnetized neutron stars. The equation of state for the DM admixed neutron star is calculated using the relativistic mean-field model with the inclusion of a density-dependent magnetic field. Several macroscopic properties, such as mass, radius, particle fractions, tidal deformability, and the f-mode frequency, are calculated with different magnetic field strengths and DM configurations. The equation of state is softer with the presence of DM as well as for the parallel components of the pressure and vice versa for the perpendicular one. Other macroscopic properties, such as mass, radius, tidal deformability, etc., are also affected by both DM and magnetic fields. The change in the magnitude of different neutron star observables is proportional to the amount of DM percentage and the strength of the magnetic field. We observe that the change is seen mainly in the core part of the star without affecting the crustal properties.

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References (75)

  1. K. Makishima, T. Enoto, J. S. Hiraga, T. Nakano, K. Nakazawa, S. Sakurai, M. Sasano, and H. Murakami, Phys. Rev. Lett. 112, 171102 (2014).
  2. M. G. Baring and A. K. Harding, Astrophys. J. 547, 929 (2001).
  3. D. C. Ellison, E. G. Berezhko, and M. G. Baring, Astrophys. J. 540, 292 (2000).
  4. S. K. Lander, Astrophys. J. Lett. 947, L16 (2023).
  5. K. Hu, M. G. Baring, A. K. Harding, and Z. Wadiasingh, Astrophys. J. 940, 91 (2022).
  6. J.-F. Fortin, H.-K. Guo, S. P. Harris, E. Sheridan, and K. Sinha, J. Cosmol. Astropart. Phys. 06 (2021) 036.
  7. O. Ferreira and E. S. Fraga, J. Cosmol. Astropart. Phys. 04 (2023) 012.
  8. V. M. Kaspi and A. M. Beloborodov, Annu. Rev. Astron. Astrophys. 55, 261 (2017).
  9. G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405, 279 (2005).
  10. G. Bertone and M. Fairbairn, Phys. Rev. D 77, 043515 (2008).
  11. N. F. Bell, G. Busoni, T. F. Motta, S. Robles, A. W. Thomas, and M. Virgato, Phys. Rev. Lett. 127, 111803 (2021).
  12. B. Kain, Phys. Rev. D 103, 043009 (2021).
  13. D. Rafiei Karkevandi, S. Shakeri, V. Sagun, and O. Ivanytskyi, Phys. Rev. D 105, 023001 (2022).
  14. C. Kouvaris, Phys. Rev. D 77, 023006 (2008).
  15. A. de Lavallaz and M. Fairbairn, Phys. Rev. D 81, 123521 (2010).
  16. F. Sandin and P. Ciarcelluti, Astropart. Phys. 32, 278 (2009).
  17. P. Ciarcelluti and F. Sandin, Phys. Lett. B 695, 19 (2011).
  18. J. Ellis, G. Hütsi, K. Kannike, L. Marzola, M. Raidal, and V. Vaskonen, Phys. Rev. D 97, 123007 (2018).
  19. D. Hooper and L.-T. Wang, Phys. Rev. D 69, 035001 (2004).
  20. A. Das, T. Malik, and A. C. Nayak, Phys. Rev. D 99, 043016 (2019).
  21. H. C. Das, A. Kumar, B. Kumar et al., J. Cosmol. Astropart. Phys. 01 (2021) 007.
  22. H. C. Das, A. Kumar, B. Kumar, and S. K. Patra, Galaxies 10, 14 (2022).
  23. H. C. Das, A. Kumar, S. K. Biswal, and S. K. Patra, Phys. Rev. D 104, 123006 (2021).
  24. H. C. Das, A. Kumar, and S. K. Patra, Mon. Not. R. Astron. Soc. 507, 4053 (2021).
  25. P. Routaray, H. C. Das, S. Sen, B. Kumar, G. Panotopoulos, and T. Zhao, Phys. Rev. D 107, 103039 (2023).
  26. L. L. Lopes and H. C. Das, J. Cosmol. Astropart. Phys. 05 (2023) 034.
  27. R. N. Manchester, G. B. Hobbs, A. Teoh, and M. Hobbs, Astron. J. 129, 1993 (2005).
  28. A. Broderick, M. Prakash, and J. M. Lattimer, Astrophys. J. 537, 351 (2000).
  29. M. Strickland, V. Dexheimer, and D. P. Menezes, Phys. Rev. D 86, 125032 (2012).
  30. V. Parmar, H. C. Das, M. K. Sharma, and S.  K. Patra, Phys. Rev. D 107, 043022 (2023).
  31. S. K. Patra, M. Centelles, X. Viñas et al., Phys. Rev. C 65, 044304 (2002).
  32. B. Kumar, S. K. Patra, and B. K. Agrawal, Phys. Rev. C 97, 045806 (2018).
  33. A. Kumar, H. C. Das, S. K. Biswal et al., Eur. Phys. J. C 80, 775 (2020).
  34. V. Parmar, H. C. Das, A. Kumar, M. K. Sharma, and S. K. Patra, Phys. Rev. D 105, 043017 (2022).
  35. H. C. Das, A. Kumar, and S. K. Patra, Phys. Rev. D 104, 063028 (2021).
  36. H. C. Das, A. Kumar, B. Kumar, S. K Biswal, T. Nakatsukasa, A. Li, and S. K. Patra, Mon. Not. R. Astron. Soc. 495, 4893 (2020).
  37. F. J. Fattoyev, C. J. Horowitz, J. Piekarewicz, and B. Reed, Phys. Rev. C 102, 065805 (2020).
  38. B. P. Abbott, R. Abbott, T. D. Abbott et al., Astrophys. J. 892, L3 (2020).
  39. H. T. Cromartie, E. Fonseca, S. M. Ransom et al., Nat. Astron. 4, 72 (2020).
  40. H. C. Das, A. Kumar, B. Kumar et al., Int. J. Mod. Phys. E 30, 2150088 (2021).
  41. G. Panotopoulos and I. Lopes, Phys. Rev. D 96, 083004 (2017).
  42. C. V. Flores, L. L. Lopes, L. B. Castro, and D. P. Menezes, Eur. Phys. J. C 80, 1 (2020).
  43. J. Frieben and L. Rezzolla, Mon. Not. R. Astron. Soc. 427, 3406 (2012).
  44. R. Ciolfi and L. Rezzolla, Mon. Not. R. Astron. Soc. 435, L43 (2013).
  45. M. Mariani, M. G. Orsaria, I. F. Ranea-Sandoval, and G. Lugones, Mon. Not. R. Astron. Soc. 489, 4261 (2019).
  46. N. K. Patra, T. Malik, D. Sen, T. K. Jha, and H. Mishra, Astrophys. J. 900, 49 (2020).
  47. G. H. Bordbar and M. Karami, Eur. Phys. J. C 82, 74 (2022).
  48. P.-C. Chu, X. Wang, L.-W. Chen, and M. Huang, Phys. Rev. D 91, 023003 (2015).
  49. I. A. Rather, U. Rahaman, V. Dexheimer, A. A. Usmani, and S. K. Patra, Astrophys. J. 917, 46 (2021).
  50. X.-G. Huang, M. Huang, D. H. Rischke, and A. Sedrakian, Phys. Rev. D 81, 045015 (2010).
  51. H. Müller and B. D. Serot, Nucl. Phys. A606, 508 (1996).
  52. P. Wang, Phys. Rev. C 61, 054904 (2000).
  53. A. Kumar, H. C. Das, S. K. Biswal et al., Eur. Phys. J. C 80 (2020).
  54. P. G. Reinhard, Rep. Prog. Phys. 52, 439 (1989).
  55. B. D. Serot and J. D. Walecka, Adv. Nucl. Phys. 16, 1 (1986).
  56. A. E. Nelson, S. Reddy, and D. Zhou, J. Cosmol. Astropart. Phys. 07 (2019) 012.
  57. M. Cassing, A. Brisebois, M. Azeem, and J. Schaffner-Bielich, Astrophys. J. 944, 130 (2023).
  58. G. Panotopoulos and I. Lopes, Phys. Rev. D 96, 083004 (2017).
  59. J. Fang, H. Pais, S. Pratapsi, S. Avancini, J. Li, and C. Providência, Phys. Rev. C 95, 045802 (2017).
  60. A. GOYAL, V. K. GUPTA, K. GOSWAMI, and V. TULI, Int. J. Mod. Phys. A 16, 347 (2001).
  61. S. Chakrabarty, Phys. Rev. D 54, 1306 (1996).
  62. D. Ebert, K. G. Klimenko, M. A. Vdovichenko, and A. S. Vshivtsev, Phys. Rev. D 61, 025005 (1999).
  63. G. N. Ferrari, A. F. Garcia, and M. B. Pinto, Phys. Rev. D 86, 096005 (2012).
  64. E. S. Fraga and L. F. Palhares, Phys. Rev. D 86, 016008 (2012).
  65. A. Haber, F. Preis, and A. Schmitt, Phys. Rev. D 90, 125036 (2014).
  66. A. Rabhi, H. Pais, P. K. Panda, and C. Providência, J. Phys. G 36, 115204 (2009).
  67. D. Bandyopadhyay, S. Chakrabarty, and S. Pal, Phys. Rev. Lett. 79, 2176 (1997).
  68. R. Mallick and S. Schramm, Phys. Rev. C 89, 045805 (2014).
  69. R. H. Casali, L. B. Castro, and D. P. Menezes, Phys. Rev. C 89, 015805 (2014).
  70. M. Mariani, L. Tonetto, M. C. Rodríguez, M. O. Celi, I. F. Ranea-Sandoval, M. G. Orsaria, and A. Pérez Martínez, Mon. Not. R. Astron. Soc. 512, 517 (2022).
  71. R. C. Tolman, Phys. Rev. 55, 364 (1939).
  72. J. R. Oppenheimer and G. M. Volkoff, Phys. Rev. 55, 374 (1939).
  73. M. C. Miller, F. K. Lamb, A. J. Dittmann et al., Astrophys. J. 887, L24 (2019).
  74. M. C. Miller, F. K. Lamb, A. J. Dittmann et al., Astrophys. J. 918, L28 (2021).
  75. T. Hinderer, Astrophys. J. 677, 1216 (2008).

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Phys. Rev. D 108, 083003– Published 2 October, 2023
  • Received 5 July 2023
  • Accepted 12 September 2023
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