\begin{document}$ f(Q) $\end{document} gravity framework. This approach provides new insights into the dynamics of compact stars and the role of dark matter in their structure. We derive the metric potential for compact stellar configurations and calculate the associated unknown parameters. Analyzing the physical properties of the compact star PSR J1614-2230 across various values of k, we find that the derived interior solutions for anisotropic stars satisfy all essential physical conditions, thereby confirming the robustness and stability of the proposed model."> Impact of the Bose-Einstein density profile on anisotropic compact stars under f (Q) gravity -
  • [1]

    M. Ruderman, Class. Ann. Rev. Astron. Astrophys.10, 427 (1972)

  • [2]

    L. Herrera and N.O. Santos, Phys. Rep.286, 53 (1997)

  • [3]

    S. K. M. Hossein, F. Rahaman, J. Naskaret al., Int. J. Mod. Phys. D21, 1250088 (2012)

  • [4]

    M. Kalam, F. Rahaman, S. Mollaet al., Astrophys. Space Sci.349, 865 (2014)

  • [5]

    B. C. Paul and R. Deb, Astrophys. Space Sci.354, 421 (2014)

  • [6]

    E. Witten, Phys. Rev. D30, 272 (1984)

  • [7]

    K. S. Cheng, Z. G. Dai, and T. Lu, Int. J. Mod. Phys. D7, 139 (1998)

  • [8]

    F. Rahaman, K. Chakraborty, P. K. F. Kuhfittiget al., Eur. Phys. J. C74, 3126 (2014)

  • [9]

    K. Bamba, S. Nojiri, and S. D. Odintsov, Phys. Lett. B698, 451 (2011)

  • [10]

    A. V. Astashenok and S. Capozziello, JCAP2013, 040 (2013)

  • [11]

    A. V. Astashenok, S. Capozziello, and S. D. Odintsov, Phys. Lett. B742, 160 (2015)

  • [12]

    A. V. Astashenok, S. Capozziello, and S. D. Odintsov, Astrophys. and Space Sci.355, 333 (2015)

  • [13]

    S. Capozziello1, M. D. Laurentis, R. Farinelliet al., Phys. Rev. D93, 023501 (2016)

  • [14]

    A. V. Astashenok, S. D. Odintsov, and A. de la Cruz-Dombriz, Class. Quantum Grav.34, 205008 (2017)

  • [15]

    A. V. Astashenok and S. D. Odintsov, Mon. Not. R. Astron. Soc.493, 78 (2020)

  • [16]

    G. G. L. Nashed and S. Capozziello, Eur. Phys. J. C81, 481 (2021)

  • [17]

    K. Numajiri, Y. X. Cui, T. Katsuragawaet al., Phys. Rev. D107, 104019 (2023)

  • [18]

    G. G. L. Nashed and S. Nojiri, Eur. Phys. J. C83, 68 (2023)

  • [19]

    Y. X. Cui, Z. Yan, K. Numajiriet al., Phys. Rev. D110, 084028 (2024)

  • [20]

    Y. Xu, T. Harko, S. Shahidiet al., Eur. Phys. J. C80, 449 (2020)

  • [21]

    S. Bhattacharjee and P. K. Sahoo, Eur. Phys. J. C80, 289 (2020)

  • [22]

    N. Godani and G. C. Samanta, Int. J. Geom. Meth. Mod. Phys.18, 2150134 (2021)

  • [23]

    V. Venkatesha, C. C. Chalavadi, N. S. Kavyaet al., New Astron.105, 102090 (2023)

  • [24]

    C. C. Chalavadi, N. S. Kavya, and V. Venkatesha, Eur. Phys. J. Plus138, 1 (2023)

  • [25]

    C. C. Chalavadi, V. Venkatesha, N. S. Kavyaet al., Commun. Theor. Phys.76, 025403 (2024)

  • [26]

    C. C. Chalavadi and V. Venkatesha, Eur. Phys. Lett146, 39001 (2024)

  • [27]

    V. Venkatesha, C. C. Chalavadi, and A. Malik, Eur. Phys. J. C84, 834 (2024)

  • [28]

    C. C. Chalavadi, V. Venkatesha, and A. Malik, Nucl. Phys. B1006, 116644 (2024)

  • [29]

    C. C. Chalavadi, V. Venkatesha, and H. A. Kumara, ADP536, 2400233 (2024)

  • [30]

    H. Weyl, Sitzungsber. Preuss. Akad. Wiss26, 465 (1918)

  • [31]

    A. Einstein, Sitzungsber. Preuss. Akad. Wiss154, 1918 (1918)

  • [32]

    E. Cartan, Ann. Ec. Norm.40, 325 (1923)

  • [33]

    R. Weitzenböck,Invariantentheorie(P. Noordhoff Groningen, 1923)

  • [34]

    J. B. Jiménez, L. Heisenberg, and T. Koivisto, Phys. Rev. D98, 044048 (2018)

  • [35]

    J. B. Jiménez, L. Heisenberg, and T. Koivisto, Universe5, 173 (2019)

  • [36]

    I. Soudi, G. Farrugia, J. L. Saidet al., Phys. Rev. D100, 044008 (2019)

  • [37]

    R. Lazkoz, F. S. N. Lobo, M. Ortiz-Banoset al., Phys. Rev. D100, 104027 (2019)

  • [38]

    B. J. Barros, T. Barreiro, T. Koivistoet al., Phys. Dark Univ.30, 100616 (2020)

  • [39]

    I. Ayuso, R. Lazkoz, and V. Salzano, Phys. Rev. D103, 063505 (2021)

  • [40]

    S. Mandal and P. K. Sahoo, Phys. Lett. B823, 136786 (2021)

  • [41]

    L. Atayde and N. Frusciante, Phys. Rev. D104, 064052 (2021)

  • [42]

    N. Frusciante, Phys. Rev. D103, 044021 (2021)

  • [43]

    F. K. Anagnostopoulos, V. Gakis, E. N. Saridakiset al., Eur. Phys. J. C83, 58 (2023)

  • [44]

    Q. Wang, X. Ren, Y. F. Caiet al., Astrophys. J974, 7 (2024)

  • [45]

    W. Wang, K. Hu, and T. Katsuragawa, arXiv: 2412.17463

  • [46]

    S. Mandal, G. Mustafa, Z. Hassanet al., Phys. Dark Unv.35, 100934 (2022)

  • [47]

    S. K. Maura, G. Mustafa, M. Govenderet al., JCAP2022, 003 (2022)

  • [48]

    S. Kaur, S. K. Maurya, and S. Shukla, Phys. scripta98, 105304 (2023)

  • [49]

    P. Bhar, S. Pradhan, A. Maliket al., Eur. Phys. J. C83, 646 (2023)

  • [50]

    P. Bhar, A. Malik, and A. Almas, Chin. J. Phys.88, 839 (2024)

  • [51]

    M. Z. Gul, S. Rani, M. Adeelet al., Eur. Phys. J. C84, 8 (2024)

  • [52]

    A. Errehymy, S. K. Maurya, K. Boshkayevet al., Phys. Dark Unv.46, 101622 (2024)

  • [53]

    P. Bhar, Fortsch. der. Phys.72, 2300183 (2024)

  • [54]

    M. A. Alwan, T. Inagaki, B. Mishraet al., JCAP2024, 011 (2024)

  • [55]

    S. K. Maurya, A. Ashraf, F. A. Khayariet al., Eur. Phys. J. C84, 986 (2024)

  • [56]

    V. C. Rubin, Jr. W. K. Ford, and N. Thonnard, Astrophys. J.238, 471 (1980)

  • [57]

    F. Zwicky, Helv. Phys. Acta6, 110 (1933)

  • [58]

    P. A. R. Adeet al. (Planck Collaboration), A & A571, A16 (2014)

  • [59]

    Bo se, Zeitschrift für Physik26, 178 (1924)

  • [60]

    E. Albert,Quantentheorie des einatomigen idealen Gases, 10.7., 1924

  • [61]

    E. Albert,Quantentheorie des einatomigen idealen Gases, 2. Abhandlung, 8.1.,1925

  • [62]

    Q. Chen, J. Stajic, S. Tanet al., Phys. Rep.412, 1 (2005)

  • [63]

    S. J. Sin, Phys. Rev. D50, 3650 (1994)

  • [64]

    S. U. Ji and S. J. Sin, Phys. Rev. D50, 3655 (1994)

  • [65]

    W. Hu, R. Barkana, and A. Gruzinov, Phys. Rev. Lett.85, 1158 (2000)

  • [66]

    C. G. Boehmer and T. Harko, JCAP06, 025 (2007)

  • [67]

    J. W. Lee, Phys. Lett. B681, 118 (2009)

  • [68]

    J. W. Lee and S. Lim, JCAP1001, 007 (2010)

  • [69]

    T. Harko, JCAP1105, 022 (2011)

  • [70]

    V. H. Robles and T. Matos, Mon. Not. R. Astron. Soc.422, 282 (2012)

  • [71]

    F. S. Guzman, F. D. Lora-Clavijo, J. J. Gonzalez-Avileset al., Phys. Rev. D89, 063507 (2014)

  • [72]

    T. Harko and E. J. M. Madarassy, JCAP01, 020 (2012)

  • [73]

    P. H. Chavanis, Phys. Rev. D84, 043531 (2011)

  • [74]

    P. H. Chavanis and L. Delfini, Phys. Rev. D84, 043532 (2011)

  • [75]

    N. K. Glendenning,Compact Stars, Nuclear Physics, Particle Physics and General Relativity(Springer, New York, 2012)

  • [76]

    S. Sarkar, N. Sarkar, P. Rudraet al., Eur. Phys. J C83, 1005 (2023)

  • [77]

    S. Aktar, K. N. Singh, P. Bharet al., Chin. J Phys.89, 1188 (2024)

  • [78]

    S. K. Maurya, A. Errehymy, G. E. Vîlcuet al., Class. Quantum Grav.41, 115009 (2024)

  • [79]

    P. H. Chavanis and T. Harko, Phys. Rev. D86, 064011 (2012)

  • [80]

    C. J. Pethick, T. Schäfer, and A. Schwenk, arXiv: 1507.05839

  • [81]

    M. E. Mosquera, O. Civitarese, O. G. Benvenutoet al., Phys. Lett. B683, 119 (2010)

  • [82]

    X. Y. Li, T. Harko, and K. S. Cheng, JCAP2012, 001 (2012)

  • [83]

    W. Wang, H. Chen, and T. Katsuragawa, Phys. Rev. D105, 024060 (2022)

  • [84]

    F. D'Ambrosio, S. D. B. Fell, L. Heisenberget al., Phys. Rev. D105, 024042 (2022)

  • [85]

    H. A. Buchdahl, Phys. Rev.116, 1027 (1959)

  • [86]

    L. Herrera, Phys. Lett. A165, 206 (1992)

  • [87]

    S. Chandrasekhar, Phys. Rev. Lett.12, 114 (1964)

Baidu
map