Nuclear Dipole Response in the Finite-Temperature Relativistic Time Blocking Approximation
Herlik Wibowo, Elena Litvinova

TL;DR
This paper extends the relativistic time blocking approximation to finite temperatures, enabling detailed study of nuclear dipole responses and low-energy modes in thermally excited nuclei, relevant for astrophysical processes.
Contribution
It introduces a finite-temperature generalization of the RTBA using Matsubara Green's functions, connecting high-energy meson effects with low-energy nuclear responses in a self-consistent framework.
Findings
Landau damping dominates temperature evolution of strength distribution.
PVC effects are strong at moderate temperatures.
High temperatures reinforce low-energy collective modes.
Abstract
The radiative neutron capture reaction rates of the r-process nucleosynthesis are immensely affected by the microscopic structure of the low-energy spectra of compound nuclei. The relativistic (quasiparticle) time blocking approximation (R(Q)TBA) has successfully provided a good description of the low-energy strength, in particular, the strength associated with pygmy dipole resonance, describing transitions from and to the nuclear ground state. The finite-temperature generalization of this method is designed for thermally excited compound nuclei and has the potential to enrich the fine structure of the dipole strength, especially in the low-energy region. The finite-temperature RTBA equations are derived using the Matsubara Green's function formalism. We show that with the help of a temperature-dependent projection operator on the subspace of the imaginary time it is possible to reduce…
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