Author

Panda, R.N.

INSPIRE profile2013759 ORCID0000-0001-5296-5187

3 papers·203 citations in this corpus

	Paper	Category
Apr 13, 2015#71504.02682	Quest of $^{37} M g$ halo structure using Glauber model and microscopic relativistic mean field densities Mahesh K. Sharma · R. N. Panda · Manoj K. Sharma · S. K. Patra	nucl-th	PRC	27
Sep 28, 2010#6*1009.5024	Application of relativistic mean field and effective field theory density to calculate scattering observables for Ca isotopes M. Bhuyan🇮🇳 · R. N. Panda🇮🇳 · T. R. Routray🇮🇳 · S. K. Patra🇮🇳	nucl-th	PRC	6
Jun 23, 2009#4*0906.3797	Formation of neutron-rich and superheavy elements in astrophysical objects S.K. Patra🇮🇳 · R.N. Panda🇮🇳	nucl-th	PRC	29

Quest of $^{37} M g$ halo structure using Glauber model and microscopic relativistic mean field densities
Mahesh K. Sharma · R. N. Panda · Manoj K. Sharma · S. K. Patra
Apr 13, 2015#7nucl-thPRC27 citations
Application of relativistic mean field and effective field theory density to calculate scattering observables for Ca isotopes
M. Bhuyan🇮🇳 · R. N. Panda🇮🇳 · T. R. Routray🇮🇳 · S. K. Patra🇮🇳
Sep 28, 2010#6*nucl-thPRC6 citations
Formation of neutron-rich and superheavy elements in astrophysical objects
S.K. Patra🇮🇳 · R.N. Panda🇮🇳
Jun 23, 2009#4*nucl-thPRC29 citations

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Panda, R.N.

Quest of 37Mg halo structure using Glauber model and microscopic relativistic mean field densities

Application of relativistic mean field and effective field theory density to calculate scattering observables for Ca isotopes

Formation of neutron-rich and superheavy elements in astrophysical objects

Quest of $^{37} M g$ halo structure using Glauber model and microscopic relativistic mean field densities