A. Kumar, H. C. Das, S. K. Biswal, B. Kumar, and S. K. Patra,"Warm dense matter and cooling of supernovae remnants", European Physics Journal C, vol.80, pp.775, European 2020, https://doi.org/10.1140/epjc/s10052-020-8353-4       Article

B. Kumar,"Neutron skins of heavy nuclei and tidal deformability of neutron star", in JPS Conference, vol.31, pp.011052, JPS, ., August 2020, https://journals.jps.jp/doi/10.7566/JPSCP.31.011052       Inproceedings

K. C. Naik, R. N. Panda, B. Kumar, and S. K. Patra,"Recent parametrization in Relativistic Mean-Field Formalism", Nuclear Structure Physics, ch.3, pp.67, CRC Press, . 2020, https://doi.org/10.1201/9780429288647       Inbook

B. Kumar and P. Landry,"Inferring Neutron Star Properties from GW170817 with Universal Relations", Physical Review D, vol.99, pp.123026, American Physical Society, June 2019, DOI: 10.1103/PhysRevD.99.123026       Article

P. Landry and B. Kumar,"Constraints on the moment of inertia of psr j0737-3039a from gw170817", Astrophysical Journal Letters, vol.868, no.2, IOP, November 2018, 10.3847/2041-8213/aaee76       Article

T. Malik, N. Alam, M. Fortin, C. Providência, B. K. Agrawal, T. K. Jha, B. Kumar, and S. K. Patra,"Gw170817: constraining the nuclear matter equation of state from the neutron star tidal deformability", Physical Review C, vol.98, no.3, American Physical Society 2018, 10.1103/physrevc.98.035804       Article

B. Kumar, S. K. Patra, and B. K. Agrawal,"New relativistic effective interaction for finite nuclei, infinite nuclear matter, and neutron stars", Physical Review C, vol.97, no.4, American Physical Society 2018, 10.1103/physrevc.97.045806       Article

M. Panigrahi, R. N. Panda, B. Kumar, and S. K. Patra,"Decay properties and reaction dynamics of zirconium isotopes in the relativistic mean-field model", International journal of modern physics e, vol.27, no.2, World Scientific 2018, 10.1142/s021830131850012x       Article

M. Ikram, A. Rather, A., B. Kumar, and S. K. Patra,"Theoretical studies on structural and decay properties of Z = 119 superheavy nuclei", Arxiv, Cornell University, May 2018, https://arxiv.org/abs/1709.07311       Article

A. Quddus, G. Panotopoulos, B. Kumar, S. Ahmad, and S. K. Patra,"Properties of a neutron star in the presence of dark matter", in DAE Nuclear Physics Proceeding, vol.63, . 2018, http://sympnp.org/proceedings/63/C27.pdf       Inproceedings