activity
19972026
most citedGamow-Teller strength distributions at finite temperatures and electron capture in stellar environments

74 citations · 195 across the 17 of their papers we have counts for

collaborators

17 papers

nucl-th2026

Reentrance of proton-neutron pairing in hot nuclear systems

T. Vu Dong, Alan A. Dzhioev, A. I. Vdovin +1

We develop a generalized finite-temperature proton-neutron BCS framework using the superoperator formalism, incorporating both isovector and isoscalar monopole pairing channels. Nu…

nucl-th2023★ 5 cited

Neutrino spectrum and energy loss rates due to weak processes on hot Fe in pre-supernova environment

Alan A. Dzhioev, A. V. Yudin, N. V. Dunina-Barkovskaya +1

Applying TQRPA calculations of Gamow--Teller strength functions in hot nuclei, we compute the (anti)neutrino spectra and energy loss rates arising from weak processes on hot $^{56}…

nucl-th2016★ 2 cited

Neutrino Processes with Hot Nuclei in Supernovae

Alan A. Dzhioev, A. I. Vdovin

In this paper, we calculate cross sections for charged-current neutrino-nucleus processes occuring under presupernova conditions. To treat thermal effects we extend self-consistent…

nucl-th2016★ 22 cited

Thermal QRPA with Skyrme interactions and supernova neutral-current neutrino-nucleus reactions

Alan A. Dzhioev, A. I. Vdovin, G. Martínez-Pinedo +2

The Thermal Quasiparticle Random-Phase Approximation is combined with the Skyrme energy density functional method (Skyrme-TQRPA) to study the response of a hot nucleus to an extern…

nucl-th2015★ 14 cited

Neutrino absorption by hot nuclei in supernova environments

Alan A. Dzhioev, A. I. Vdovin, J. Wambach

Using the thermal quasiparticle random phase approximation, we study the process of neutrino and antineutrino capture on hot nuclei in supernova environments. For the sample nuclei…

nucl-th2014★ 21 cited

Inelastic neutrino scattering off hot nuclei in supernova environments

Alan A. Dzhioev, A. I. Vdovin, J. Wambach +1

We study inelastic neutrino scattering off hot nuclei for temperatures relevant under supernova conditions. The method we use is based on the quasiparticle random phase approximati…