17 citations · 49 across the 12 of their papers we have counts for
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Energy Rates Due to Weak Decay Rates of Vanadium Isotopes in Stellar Environment
Ramoona Shehzadi, Jameel-Un Nabi, Huma Ali
The neutrino cooling and gamma heating rates are considered as an important input needed to study the final phases of the evolution of high-mass stars. The weak-interaction mediate…
Neutrino cooling rates due to nickel isotopes for presupernova evolution of massive stars
Jameel-Un Nabi, Ramoona Shehzadi, Muhammad Majid
Simulation studies indicate that weak interaction rates on nickel isotopes play a crucial role in determining the electron-to-baryon ratio within the stellar interior during the la…
Lepton capture rates due to isotopes of vanadium in astrophysical environment
Ramoona Shehzadi, Jameel-Un Nabi, Fakeha Farooq
Lepton (electron and positron) capture rates on iron-regime nuclei are an essential element for modeling the late stages in the evolution of massive stars that end as core-collapse…
-decay properties of some astrophysically important Sc-isotopes
Fakeha Farooq, Jameel-Un Nabi, Ramoona Shehzadi
In the late progressive stages of heavy stars, electron capture and -decay are the governing processes. The weak rates are essential inputs for modeling the stages of high-m…
Lepton emission rates of 43-64V isotopes under stellar conditions
Ramoona Shehzadi, Jameel-Un Nabi, Fakeha Farooq
In astrophysical conditions prevalent during the late times of stellar evolution, lepton ( and ) emission processes compete with the corresponding lepton capture processe…
-Decay Properties of Neutron-rich Yttrium Isotopes
Fakeha Farooq, Jameel-Un Nabi, Ramoona Shehzadi
In this study, we have reported key nuclear properties of weak -decay processes on Yttrium isotopes for the mass number range . This mass region is important in a…
Beta decay and electron capture rates on manganese isotopes in astrophysical environments
R. Shehzadi, J. -U. Nabi, F. Farooq
The isotopes of manganese in the mass range A equal to 53 to 63 are abundant in the core material of high mass stars and are believed to be of prime importance in the progression o…
Validity of Brink Axel Hypothesis for calculations of allowed stellar weak rates of heavy nuclei
Fakeha Farooq, Jameel-Un Nabi, Ramoona Shehzadi
The knowledge of beta decay transitional probabilities and GamowTeller (GT) strength functions from highly excited states of nuclides is of particular importance for applications t…
Gamow-Teller strength distributions and neutrino energy loss rates due to chromium isotopes in stellar matter
Jameel-Un Nabi, Ramoona Shehzadi, Muhammad Fayaz
Gamow-Teller transitions in isotopes of chromium play a consequential role in the presupernova evolution of massive stars. -decay and electron capture rates on chromium isotopes…