Author

Behera, Bivash R.

13 papers·227 citations in this corpus

	Paper	Category
Sep 2, 2020#62009.00427	Constraining Nuclear Symmetry Energy parameters from Neutron skin thickness of $^{48}$ Ca S. K. Tripathy · D. Behera · T. R. Routray · B. Behera	nucl-th	—	5
Jun 30, 2020#52006.15430	Constraints from GW170817 on the bulk viscosity of neutron star matter and the r-mode instability T. R. Routray🇮🇳 · S. P. Pattnaik🇮🇳 · C. Gonzalez-Boquera🇪🇸 · X. Viñas🇪🇸 · M. Centelles🇪🇸 · B. Behera🇮🇳	nucl-th	—	5
Apr 30, 2020#72004.14205	Nuclear Symmetry Energy and Neutron Skin Thickness of $^{208} P b$ using a finite range effective interaction D. Behera · S. K. Tripathy · T. R. Routray · B. Behera	nucl-th	Phys.Scripta	13
Dec 21, 2017#11712.07273	Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction S. P. Pattnaik🇮🇳 · T. R. Routray🇮🇳 · X. Viñas🇪🇸 · D. N. Basu🇮🇳 · M. Centelles🇪🇸 · K. Madhuri🇮🇳 · B. Behera🇮🇳	nucl-th	J.Phys.G	15
Apr 13, 2017#91704.03860	Deformation properties with a finite range simple effective interaction B. Behera · X. Viñas · T. R. Routray · L. M. Robledo · M. Centelles · S. P. Pattnaik	nucl-th	J.Phys.G	25
Jul 29, 2016#51607.08531	Exact versus Taylor-expanded energy density in the study of the neutron star crust-core transition T. R. Routray · X. Viñas · D. N. Basu · S. P. Pattnaik · M. Centelles · L. Robledo · B. Behera	nucl-th	J.Phys.G	26
Oct 13, 2015#151510.02924	No influence of a N=126 Neutron Shell Closure in Fission Fragment Mass Distributions A. Chaudhuri · T. K. Ghosh · K. Banerjee · S. Bhattacharya · Jhilam Sadhukhan · S. Kundu · C. Bhattacharya · J. K. Meena · G. Mukherjee · A. K. Saha · Md. A. Asgar · A. Dey · S. Manna · R. Pandey · T. K. Rana · P. Roy · T. Roy · V. Srivastava · P. Bhattacharya · D. C. Biswas · B. N. Joshi · K. Mahata · A. Shrivastava · R. P. Vind · S. Pal	↳ nucl-ex	PRC	18
Sep 21, 2015#31509.05666	Influence of vibrational excitation on surface diffuseness of inter-nuclear potential: study through heavy-ion quasi-elastic scattering at deep subbarrier energies Gurpreet Kaur · B.R. Behera · A. Jhingan · P. Sugathan · K. Hagino	nucl-th	PRC	1
Jan 13, 2015#51501.02651	Study of spin polarized nuclear matter and finite nuclei with finite range simple effective interaction B. Behera🇮🇳 · X. Viñas🇪🇸 · T. R. Routray🇮🇳 · M. Centelles🇪🇸	nucl-th	J.Phys.G	21
Feb 15, 2013#6*1302.3421	Simple effective interaction: Infinite nuclear matter and finite nuclei B. Behera · X. Vinas · M. Bhuyan · T. R. Routray · B. K. Sharma · S. K. Patra	nucl-th	J.Phys.G	37
Aug 22, 2012#3*1208.4236	An effective Nuclear Model: from Nuclear Matter to Finite Nuclei T.R.Routray🇮🇳 · X.Vinas🇪🇸 · S.K. Tripathy🇮🇳 · M.Bhuyan🇮🇳 · S.K.Patra🇮🇳 · B.Behera🇮🇳	nucl-th	J.Phys.Conf.Ser.	4
Aug 10, 2011#3*1108.1930	Neutron-proton effective mass splitting and thermal evolution in neutron rich matter B.Behera🇮🇳 · T.R.Routray🇮🇳 · S.K.Tripathy🇮🇳	nucl-th	J.Phys.G	34
Dec 8, 2009#1*0912.1205	Proton radioactivity with a Yukawa effective interaction T. R. Routray🇮🇳 · S. K. Tripathy🇮🇳 · B. B. Dash🇮🇳 · B. Behera🇮🇳 · D. N. Basu🇮🇳	nucl-th	EPJA	23

Constraining Nuclear Symmetry Energy parameters from Neutron skin thickness of $^{48}$ Ca
S. K. Tripathy · D. Behera · T. R. Routray · B. Behera
Sep 2, 2020#6nucl-th5 citations
Constraints from GW170817 on the bulk viscosity of neutron star matter and the r-mode instability
T. R. Routray🇮🇳 · S. P. Pattnaik🇮🇳 · C. Gonzalez-Boquera🇪🇸 · X. Viñas🇪🇸 · M. Centelles🇪🇸 · B. Behera🇮🇳
Jun 30, 2020#5nucl-th5 citations
Nuclear Symmetry Energy and Neutron Skin Thickness of $^{208} P b$ using a finite range effective interaction
D. Behera · S. K. Tripathy · T. R. Routray · B. Behera
Apr 30, 2020#7nucl-thPhys.Scripta13 citations
Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction
S. P. Pattnaik🇮🇳 · T. R. Routray🇮🇳 · X. Viñas🇪🇸 · D. N. Basu🇮🇳 · M. Centelles🇪🇸 · K. Madhuri🇮🇳 · B. Behera🇮🇳
Dec 21, 2017#1nucl-thJ.Phys.G15 citations
Deformation properties with a finite range simple effective interaction
B. Behera · X. Viñas · T. R. Routray · L. M. Robledo · M. Centelles · S. P. Pattnaik
Apr 13, 2017#9nucl-thJ.Phys.G25 citations
Exact versus Taylor-expanded energy density in the study of the neutron star crust-core transition
T. R. Routray · X. Viñas · D. N. Basu · S. P. Pattnaik · M. Centelles · L. Robledo · B. Behera
Jul 29, 2016#5nucl-thJ.Phys.G26 citations
No influence of a N=126 Neutron Shell Closure in Fission Fragment Mass Distributions
A. Chaudhuri · T. K. Ghosh · K. Banerjee · S. Bhattacharya · Jhilam Sadhukhan · S. Kundu · C. Bhattacharya · J. K. Meena · G. Mukherjee · A. K. Saha · Md. A. Asgar · A. Dey · S. Manna · R. Pandey · T. K. Rana · P. Roy · T. Roy · V. Srivastava · P. Bhattacharya · D. C. Biswas · B. N. Joshi · K. Mahata · A. Shrivastava · R. P. Vind · S. Pal
Oct 13, 2015#15↳ nucl-exPRC18 citations
Influence of vibrational excitation on surface diffuseness of inter-nuclear potential: study through heavy-ion quasi-elastic scattering at deep subbarrier energies
Gurpreet Kaur · B.R. Behera · A. Jhingan · P. Sugathan · K. Hagino
Sep 21, 2015#3nucl-thPRC1 citation
Study of spin polarized nuclear matter and finite nuclei with finite range simple effective interaction
B. Behera🇮🇳 · X. Viñas🇪🇸 · T. R. Routray🇮🇳 · M. Centelles🇪🇸
Jan 13, 2015#5nucl-thJ.Phys.G21 citations
Simple effective interaction: Infinite nuclear matter and finite nuclei
B. Behera · X. Vinas · M. Bhuyan · T. R. Routray · B. K. Sharma · S. K. Patra
Feb 15, 2013#6*nucl-thJ.Phys.G37 citations
An effective Nuclear Model: from Nuclear Matter to Finite Nuclei
T.R.Routray🇮🇳 · X.Vinas🇪🇸 · S.K. Tripathy🇮🇳 · M.Bhuyan🇮🇳 · S.K.Patra🇮🇳 · B.Behera🇮🇳
Aug 22, 2012#3*nucl-thJ.Phys.Conf.Ser.4 citations
Neutron-proton effective mass splitting and thermal evolution in neutron rich matter
B.Behera🇮🇳 · T.R.Routray🇮🇳 · S.K.Tripathy🇮🇳
Aug 10, 2011#3*nucl-thJ.Phys.G34 citations
Proton radioactivity with a Yukawa effective interaction
T. R. Routray🇮🇳 · S. K. Tripathy🇮🇳 · B. B. Dash🇮🇳 · B. Behera🇮🇳 · D. N. Basu🇮🇳
Dec 8, 2009#1*nucl-thEPJA23 citations

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