10 papers
Predictions for Identified Hadron (, and ) Production and Collective Dynamics in Oxygen-Oxygen Collisions at = 7 TeV with EPOS4, AMPT-SM, and Angantyr in Pythia 8
Rabia Bashir, Ramoona Shehzadi, M. U. Ashraf +1
We study the dynamics of identified hadrons (, and ) production in collisions at TeV using recently updated versi…
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 $β^\pm$-decay are the governing processes. The weak rates are essential inputs for modeling the stages of high-…
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…