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NNNLO pressure of cold quark matter: leading logarithm
At high baryon chemical potential μB, the equation of state of QCD allows a weak-coupling expansion in the QCD coupling αs. The result is currently known up to and including the full next-to-next-to-leading order αs2. Starting at this order, the computations are complicated by the modification of pa...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2018
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.121.202701 http://cds.cern.ch/record/2645125 |
_version_ | 1780960427691212800 |
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author | Gorda, Tyler Kurkela, Aleksi Romatschke, Paul Säppi, Matias Vuorinen, Aleksi |
author_facet | Gorda, Tyler Kurkela, Aleksi Romatschke, Paul Säppi, Matias Vuorinen, Aleksi |
author_sort | Gorda, Tyler |
collection | CERN |
description | At high baryon chemical potential μB, the equation of state of QCD allows a weak-coupling expansion in the QCD coupling αs. The result is currently known up to and including the full next-to-next-to-leading order αs2. Starting at this order, the computations are complicated by the modification of particle propagation in a dense medium, which necessitates nonperturbative treatment of the scale αs1/2μB. We apply a hard-thermal-loop scheme for capturing the contributions of this scale to the weak-coupling expansion, and we use it to determine the leading-logarithm contribution to next-to-next-to-next-to-leading order: αs3ln2αs. This result is the first improvement to the equation of state of massless cold quark matter in 40 years. The new term is negligibly small and thus significantly increases our confidence in the applicability of the weak-coupling expansion. |
id | cern-2645125 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2018 |
record_format | invenio |
spelling | cern-26451252022-08-10T12:28:23Zdoi:10.1103/PhysRevLett.121.202701http://cds.cern.ch/record/2645125engGorda, TylerKurkela, AleksiRomatschke, PaulSäppi, MatiasVuorinen, AleksiNNNLO pressure of cold quark matter: leading logarithmnucl-thNuclear Physics - Theoryastro-ph.HEAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyAt high baryon chemical potential μB, the equation of state of QCD allows a weak-coupling expansion in the QCD coupling αs. The result is currently known up to and including the full next-to-next-to-leading order αs2. Starting at this order, the computations are complicated by the modification of particle propagation in a dense medium, which necessitates nonperturbative treatment of the scale αs1/2μB. We apply a hard-thermal-loop scheme for capturing the contributions of this scale to the weak-coupling expansion, and we use it to determine the leading-logarithm contribution to next-to-next-to-next-to-leading order: αs3ln2αs. This result is the first improvement to the equation of state of massless cold quark matter in 40 years. The new term is negligibly small and thus significantly increases our confidence in the applicability of the weak-coupling expansion.At high baryon chemical potential mu_B, the equation of state of QCD allows a weak-coupling expansion in the QCD coupling alpha_s. The result is currently known up to and including the full next-to-next-to-leading order (NNLO) alpha_s^2. Starting at this order, the computations are complicated by the modification of particle propagation in a dense medium, which necessitates non-perturbative treatment of the scale Sqrt(alpha_s)*mu_B. In this work, we apply a Hard-Thermal-Loop scheme for capturing the contributions of this scale to the weak-coupling expansion, and use it to determine the leading-logarithm contribution to NNNLO: alpha_s^3 (ln alpha_s)^2. This result is the first improvement to the equation of state of massless cold quark matter in 40 years. The new term is negligibly small, and thus significantly increases our confidence in the applicability of the weak-coupling expansion.arXiv:1807.04120CERN-TH-2018-230HIP-2018-13/THoai:cds.cern.ch:26451252018-07-11 |
spellingShingle | nucl-th Nuclear Physics - Theory astro-ph.HE Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology Gorda, Tyler Kurkela, Aleksi Romatschke, Paul Säppi, Matias Vuorinen, Aleksi NNNLO pressure of cold quark matter: leading logarithm |
title | NNNLO pressure of cold quark matter: leading logarithm |
title_full | NNNLO pressure of cold quark matter: leading logarithm |
title_fullStr | NNNLO pressure of cold quark matter: leading logarithm |
title_full_unstemmed | NNNLO pressure of cold quark matter: leading logarithm |
title_short | NNNLO pressure of cold quark matter: leading logarithm |
title_sort | nnnlo pressure of cold quark matter: leading logarithm |
topic | nucl-th Nuclear Physics - Theory astro-ph.HE Astrophysics and Astronomy hep-ph Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1103/PhysRevLett.121.202701 http://cds.cern.ch/record/2645125 |
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