most citedComparative study of Gamow-Teller strength distributions in the odd-odd nucleus 50V and its impact on electron capture rates in astrophysical environments

22 citations · 78 across the 6 of their papers we have counts for

collaborators

6 papers

nucl-th20116 cited

Neutrino and antineutrino energy loss rates in massive stars due to isotopes of titanium

Jameel-Un Nabi

Weak interaction rates on titanium isotopes are important during the late phases of evolution of massive stars. A search was made for key titanium isotopes from available literatur…

nucl-th201118 cited

Neutrino energy loss rates and positron capture rates on Co for presupernova and supernova physics

Jameel-Un Nabi, Muhammad Sajjad

Proton-neutron quasi-particle random phase approximation (pn-QRPA) theory has recently being used for calculation of stellar weak interaction rates of -shell nuclide with succe…

nucl-th201122 cited

Comparative study of Gamow-Teller strength distributions in the odd-odd nucleus 50V and its impact on electron capture rates in astrophysical environments

Jameel-Un Nabi, Muhammad Sajjad

Gamow-Teller (GT) strength transitions are an ideal probe for testing nuclear structure models. In addition to nuclear structure, GT transitions in nuclei directly affect the early…

nucl-th201120 cited

Gamow-Teller transitions from 24Mg and its impact on the electron capture rates in the O + Ne + Mg cores of stars

Jameel-Un Nabi, Muneeb-Ur Rahman

Electron captures on nuclei play an important role in the collapse of stellar core in the stages leading to a type-II supernova. Recent observations of subluminous Type II-P supern…

nucl-th20111 cited

Electron capture rates on titanium isotopes in stellar matter

Jameel-Un Nabi, Muhammad Sajjad, Muneeb-Ur Rahman

Electron captures are amongst the most important weak interaction rates related to the dynamics of stellar core collapse. They play a key role in the gravitational collapse of the…

nucl-th201111 cited

Stellar neutrino energy loss rates due to Mg suitable for O+Ne+Mg core simulations

Jameel-Un Nabi

Neutrino losses from proto-neutron stars play a pivotal role to decide if these stars would be crushed into black holes or explode as supernovae. Recent observations of subluminous…