Journal Articles

1. P. Thakur, T. Malik, A. Das, T. K. Jha, and C. ç. Providência, “Exploring robust correlations between
fermionic dark matter model parameters and neutron star properties: A two-fluid perspective,”  Phys.
Rev. D, vol. 109, p. 043 030, 4 Feb. 2024. doi: 10.1103/PhysRevD.109.043030.

2 P. Thakur, T. Malik, A. Das, T. K. Jha, B. K. Sharma, and C. Providência, “Feasibility of dark matter
admixed neutron star based on recent observational constraints,” 2024. arXiv: 2408.03780 [nucl-th].
 url: https://arxiv.org/abs/2408.03780.

3 P. Thakur, T. Malik, and T. K. Jha, “Towards uncovering dark matter effects on neutron star properties:
A machine learning approach,” Particles, vol. 7, no. 1, pp. 80–95, 2024, issn: 2571-712X. doi:
10.3390/particles7010005.

4 P. Thakur, B. K. Sharma, A. Ashika, S. Srivishnu, and T. K. Jha, “Influence of the symmetry energy and
σ-cut potential on the properties of pure nucleonic and hyperon-rich neutron star matter,” Phys. Rev.
C, vol. 109, p. 025 805, 2 Feb. 2024. doi: 10.1103/PhysRevC.109.025805.

5 N. K. Patra, P. Saxena, B. K. Agrawal, and T. K. Jha, “Establishing connection between neutron star
properties and nuclear matter parameters through a comprehensive multivariate analysis,” Phys. Rev. D,
vol. 108, p. 123 015, 12 Dec. 2023. doi: 10.1103/PhysRevD.108.123015.

6 P. Thakur, N. K. Patra, T. K. Jha, and T. Malik, “High-density behavior of symmetry energy and speed
of sound in the dense matter within an effective chiral model,” 2023. arXiv: 2301.12690 [nucl-th]. url: https://arxiv.org/abs/2301.12690.

7 O. P. Jyothilakshmi, P. E. S. Krishnan, P. Thakur, V. Sreekanth, and T. K. Jha, “Hyperon bulk viscosity
and r-modes of neutron stars,” Monthly Notices of the Royal Astronomical Society, vol. 516, no. 3,
pp. 3381–3388, Aug. 2022, issn: 0035-8711. doi: 10.1093/mnras/stac2360. eprint:
https://academic.oup.com/mnras/article-pdf/516/3/3381/45882806/stac2360.pdf.

8 N. K. Patra, B. K. Sharma, A. Reghunath, A. K. H. Das, and T. K. Jha, “Effect of the σ-cut potential on
the properties of neutron stars with or without a hyperonic core,” Phys. Rev. C, vol. 106, p. 055 806, 5
Nov. 2022. doi: 10.1103/PhysRevC.106.055806.

9 N. K. Patra, T. Malik, D. Sen, T. K. Jha, and H. Mishra, “An equation of state for magnetized neutron
star matter and tidal deformation in neutron star mergers,” The Astrophysical Journal, vol. 900, no. 1,
p. 49, Aug. 2020. doi: 10.3847/1538-4357/aba8fc.

10 B. K. Sharma, S. Sathees, M. K. Meghaa, and T. K. Jha, “Effect of v coupling on liquid gas phase
transition in warm asymmetric nuclear matter,” Nuclear Physics A, vol. 1002, p. 121 974, 2020, issn:
0375-9474. doi: https://doi.org/10.1016/j.nuclphysa.2020.121974.

11 T. Malik, B. K. Agrawal, J. N. De, Samaddar, S. K., Providencia, C., Mondal, C. and Jha, T. K., “Tides in merging neutron stars: Consistency of the gw170817
event with experimental data on finite nuclei,” Phys. Rev. C, vol. 99, p. 052 801, 5 May 2019. doi:
10.1103/PhysRevC.99.052801.

12 D. Sen and T. K. Jha, “Deconfinement of nonstrange hadronic matter with nucleons and ∆ baryons to
quark matter in neutron stars,” International Journal of Modern Physics D, vol. 28, no. 02, p. 1 950 040,
2019. doi: 10.1142/S0218271819500408. eprint: https://doi.org/10.1142/S0218271819500408.

13 T. Malik, N. Alam, M. Fortin, Providencia, C., Agrawal, B. K., Jha, T. K., Bharat Kumar and Patra, S. K., “GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability,” Phys. Rev. C, vol. 98, p. 035 804, 3 Sep. 2018. doi:
10.1103/PhysRevC.98.035804.

14 D. Sen, K. Banerjee, and T. K. Jha, “Properties of neutron stars with hyperon cores in parametrized
hydrostatic conditions,” International Journal of Modern Physics E, vol. 27, no. 11, p. 1 850 097, 2018.
doi: 10.1142/S0218301318500970. eprint: https://doi.org/10.1142/S0218301318500970.

15 D. Sen and T. K. Jha, “Effects of hadron–quark phase transition on properties of neutron stars,” Journal
of Physics G: Nuclear and Particle Physics, vol. 46, no. 1, p. 015 202, Dec. 2018. doi:
10.1088/1361-6471/aaf0b0.

16 T. Malik, K. Banerjee, T. K. Jha, and B. K. Agrawal, “Nuclear symmetry energy with mesonic
cross-couplings in the effective chiral model,” Phys. Rev. C, vol. 96, p. 035 803, 3 Sep. 2017. doi:
10.1103/PhysRevC.96.035803.

17 S. K. Singh, S. K. Biswal, M. Bhuyan, T. K. Jha, and S. K. Patra, “Properties of rotating neutron star,”
Journal of Nuclear Physics, Material Sciences, Radiation and Applications 3, 93 - 96, 2015. doi:
10.15415/jnp.2015.31011.

18 T. K. Jha and K. C. Panda, “Massive neutron stars and their implications,” Pramana - J Phys 82, 831–839, 2014. url: https://doi.org/10.1007/s12043-014-0736-3.

19 P. K. Das, J. Selvaganapathy, C. Sharma, T. K. Jha, and V. S. KUMAR, “Tsallis statistics and the role of a
stabilized radion in the supernovae sn1987a cooling,” International Journal of Modern Physics A, vol. 28,
no. 29, p. 1 350 152, 2013. doi: 10.1142/S0217751X13501522. eprint:
https://doi.org/10.1142/S0217751X13501522.

20 S. K. Singh, S. K. Biswal, M. Bhuyan, T. K. Jha, and S. K. Patra, “Gravitational wave from rotating
neutron star,” 2013. arXiv: 1312.5840 [astro-ph.SR]. url: https://arxiv.org/abs/1312.5840.

21 T. K. Jha, H. Mishra, and V. Sreekanth, “Bulk viscosity in a hyperonic star and r-mode instability,”
Phys. Rev. C, vol. 82, p. 025 803, 2 Aug. 2010. doi: 10.1103/PhysRevC.82.025803.

22 T. K. Jha, “‘f0(600)’ and chiral dynamics,” 2009. arXiv: 0905.4827 [nucl-th].  url:
https://arxiv.org/abs/0905.4827.

23 T. K. Jha, “From nuclear matter to neutron stars,” 2009. arXiv: 0902.0262 [nucl-th].  url:
https://arxiv.org/abs/0902.0262.

24 B. K. Sharma and T. K. Jha, “Axially-symmetric neutron stars: Implication of rapid rotation,” 2009.
arXiv: 0905.1549 [nucl-th].  url: https://arxiv.org/abs/0905.1549.

25. T. K. Jha and H. Mishra, “Constraints on nuclear matter parameters of an effective chiral model,” Phys.
Rev. C, vol. 78, p. 065 802, 6 Dec. 2008. doi: 10.1103/PhysRevC.78.065802.

26. T. K. Jha, H. Mishra, and V. Sreekanth, “Attributes of a rotating neutron star with a hyperon core,”
Phys. Rev. C, vol. 77, p. 045 801, 4 Apr. 2008. doi: 10.1103/PhysRevC.77.045801.

27. T. K. Jha, P. K. Raina, P. K. Panda, and S. K. Patra, “Neutron star matter in an effective model,” Phys.
Rev. C, vol. 74, p. 055 803, 5 Nov. 2006. doi: 10.1103/PhysRevC.74.055803.

28. M. S. Mehta, T. K. Jha, S. K. Patra, and R. K. Gupta, “Potential energy surfaces for n =z, 20ne - 112ba
nuclei,” Pramana - J Phys 62, 841–859, 2004. url: https://doi.org/10.1007/BF02706133.

29. Z. Naik, B. K. Sharma, T. K. Jha, P. Arumugam, and S. K. Patra, “Shape change in hf, w and os-isotopes:
A non-relativistic hartree-fock versus relativistic hartree approximation,” Pramana - J Phys 62, 827-839,
2004. url: https://doi.org/10.1007/BF02706132.

30. P. Sahu, T. K. Jha, K. C. Panda, and S. K. Patra, “Hot nuclear matter in asymmetry chiral sigma model,”
Nuclear Physics A, vol. 733, no. 1, pp. 169–184, 2004, issn: 0375-9474.  doi: https://doi.org/10.1016/j.nuclphysa.2003.11.061.

31. T. K. Jha, M. S. Mehta, S. K. Patra, B. K. Raj, and R. K. Gupta, “A relativistic mean-field study of magic
numbers in light nuclei from neutron to proton drip-lines.,” Pramana - J Phys 61, 517–527, 2003. url:
https://doi.org/10.1007/BF02705475.