On high-order perturbative calculations at finite density

DOI10.1016/j.nuclphysb.2016.11.023zbMath1354.81053arXiv1609.04339OpenAlexW2523504220MaRDI QIDQ505506

Saga Säppi, Paul Romatschke, Tyler Gorda, Ioan Ghişoiu, Aleksi Kurkela, Aleksi Vuorinen

Publication date: 25 January 2017

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1609.04339

zbMATH Keywords

neutron stars

Mathematics Subject Classification ID

Strong interaction, including quantum chromodynamics (81V05) Perturbative methods of renormalization applied to problems in quantum field theory (81T15) Feynman diagrams (81T18) Galactic and stellar structure (85A15) Statistical thermodynamics (82B30) Thermal quantum field theory (81T28)

Related Items (4)

Perturbative thermal QCD: formalism and applications ⋮ Structure of magnetized strange quark star in perturbative QCD ⋮ R²-gravity quark stars from perturbative QCD ⋮ Integrating by parts at finite density

Cites Work

• Finite-Temperature Field Theory
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>S</mml:mi></mml:math>-Matrix Formulation of Statistical Mechanics

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