Zobrazeno 1 - 10
of 47
pro vyhledávání: '"T. R. Routray"'
Publikováno v:
Indian Journal of Physics. 95:1225-1230
The half-life of proton radioactivity of proton emitters is investigated theoretically by using KDE0v1 Skyrme interaction. The total barrier potential in the proton radioactive nuclei is calculated as the sum of the nuclear, Coulomb and centrifugal c
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
instname
ACKNOWLEDGMENTS Useful discussions with F. Stancu are warmly acknowledged. P. Bano acknowledges the support from MANF Fellowship of UGC, India. T.R.R. gives sincere thanks to Professor B. Behera for meaningful discussions. M.C. and X.V. were partiall
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81d5d12aaa1d5bf7b0e84113e745cc85
http://hdl.handle.net/10486/704794
http://hdl.handle.net/10486/704794
Publikováno v:
Physical Review C. 104
Recent experiments performed in neutron-rich copper isotopes have revealed a crossing in the nucleus $^{75}\mathrm{Cu}$ between the $3/{2}^{\ensuremath{-}}$ and $5/{2}^{\ensuremath{-}}$ levels, which correspond to the ground state and the first excit
Publikováno v:
Springer Proceedings in Physics ISBN: 9789811590610
The finite range Simple Effective Interaction (SEI) has been constructed with minimum number of parameters that can simulate the correct trend of momentum dependence of nuclear mean field, as ascertained from the heavy-ion collision experiments at in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6934ac476cd7153e762c36eae7a6e1e7
https://doi.org/10.1007/978-981-15-9062-7_17
https://doi.org/10.1007/978-981-15-9062-7_17
We use a finite range simple effective interaction to construct nuclear equations of state for the study of the density dependence of the nuclear symmetry energy. The EoSs provide good descriptions of the nuclear symmetry energy at a subsaturation de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce893c0798fe3303767ed8d1756ec7d0
http://arxiv.org/abs/2004.14205
http://arxiv.org/abs/2004.14205
Publikováno v:
Physical Review C. 100
The properties of the core-crust transition in neutron stars are investigated using effective nuclear forces of finite range. Special attention is paid to the so-called dynamical method for locating the transition point, which, apart from the stabili
Publikováno v:
Dipòsit Digital de la UB
Universidad de Barcelona
Universidad de Barcelona
The characteristic physical properties of rotating neutron stars under the r-mode oscillation are evaluated using the finite-range simple effective interaction. Emphasis is given on examining the influence of the stiffness of both the symmetric and a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d239bf60319c83534f85bf96b65a0921
http://hdl.handle.net/2445/156042
http://hdl.handle.net/2445/156042
Publikováno v:
The European Physical Journal A. 53
The mass, radius and crustal fraction of moment of inertia in neutron stars are calculated using $\beta$ -equilibrated nuclear matter obtained from the Skyrme effective interaction. The transition density, pressure and proton fraction at the inner ed
High density behaviour of nuclear symmetry energy is studied on the basis of a stiffest density dependence of asymmetric contribution to energy per nucleon in charge neutral $n+p+e+\mu$ matter under beta equilibrium. The density dependence of nuclear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa1d322650a81cf04d421eda3267ba36
http://arxiv.org/abs/1610.06789
http://arxiv.org/abs/1610.06789
Publikováno v:
EPJ Web of Conferences, Vol 117, p 07009 (2016)
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
The nuclear mean field as a function of momentum and density is the quantity of crucial relevance in the study of nuclear matter and the equation of state can be obtained from it at momentum equals to Fermi momentum. In order to simulate the momentum