Isospin-Asymmetry Dependence of the Thermodynamic Nuclear Equation of State in Many-Body Perturbation Theory
Corbinian Wellenhofer

TL;DR
This paper investigates how the nuclear equation of state depends on isospin asymmetry at finite temperatures using chiral effective field theory and many-body perturbation theory, revealing nonanalytic behavior at low temperatures.
Contribution
It provides a detailed analysis of the isospin-asymmetry expansion in nuclear matter and uncovers divergence of higher-order terms at zero temperature, indicating nonanalytic dependence.
Findings
Higher-order expansion coefficients diverge at zero temperature.
Nonanalytic isospin-asymmetry dependence with logarithmic terms.
Finite-temperature effects on the nuclear liquid-gas phase transition.
Abstract
The computation of the thermodynamic properties of nuclear matter is a central task of theoretical nuclear physics. The nuclear equation of state is an essential quantity in nuclear astrophysics and governs the properties of neutron stars and core-collapse supernov\ae. The framework of chiral effective field theory provides the basis for the description of nuclear interactions in terms of a systematic low-energy expansion. In this thesis, we apply chiral two- and three-nucleon interactions in perturbative many-body calculations of the thermodynamic equation of state of infinite homogeneous nuclear matter. The conceptual issues that arise concerning the consistent generalization of the standard zero-temperature form of many-body perturbation theory to finite temperatures are investigated in detail. The structure of many-body perturbation theory at higher orders is examined, in particular…
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Taxonomy
TopicsNuclear physics research studies · Quantum Chromodynamics and Particle Interactions · High-pressure geophysics and materials
