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相关论文: Temperature-dependence of the QCD topological susc…

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We study the topological susceptibility in 2+1 flavor QCD above the chiral crossover transition temperature using Highly Improved Staggered Quark action and several lattice spacings, corresponding to temporal extent of the lattice,…

高能物理 - 格点 · 物理学 2016-11-29 Peter Petreczky , Hans-Peter Schadler , Sayantan Sharma

Axion cosmology needs the QCD topological susceptibility between 400 and 1100 MeV. In this range the bottom quark is inconvenient to include in lattice simulations, but not heavy enough to ignore. We estimate its effect on the…

高能物理 - 唯象学 · 物理学 2025-11-07 Bruno Högl , Guy D. Moore

In this work we compute the axion mass and, from this (exploiting a well-known relation), we also derive an expression for the QCD topological susceptibility in the finite-temperature case, both below and above the chiral phase transition…

高能物理 - 唯象学 · 物理学 2020-08-04 Salvatore Bottaro , Enrico Meggiolaro

The properties of the QCD axion are strictly related to the dependence of strong interactions on the topological parameter theta. We present a determination of the topological properties of QCD for temperatures up to around 600 MeV,…

We investigate the topological properties of $N_f = 2+1$ QCD with physical quark masses, both at zero and finite temperature. We adopt stout improved staggered fermions and explore a range of lattice spacings $a \sim 0.05 - 0.12$ fm. At…

Axions are one of the most attractive dark matter candidates. The evolution of their number density in the early universe can be determined by calculating the topological susceptibility $\chi(T)$ of QCD as a function of the temperature.…

高能物理 - 格点 · 物理学 2015-11-18 S. Borsanyi , M. Dierigl , Z. Fodor , S. D. Katz , S. W. Mages , D. Nogradi , J. Redondo , A. Ringwald , K. K. Szabo

QCD topological susceptibility at high temperature, $\chi_t(T)$, provides an important input for the estimate of the axion abundance in the present Universe. While the model independent determination of $\chi_t(T)$ should be possible from…

高能物理 - 格点 · 物理学 2016-09-21 J. Frison , R. Kitano , H. Matsufuru , S. Mori , N. Yamada

It is shown that gauge field configurations with higher topological charge modify the structure of the QCD vacuum, which is reflected in its dependence on the CP-violating topological phase $\theta$. To explore this, topological…

高能物理 - 理论 · 物理学 2020-09-09 Fabian Rennecke

In a previous paper \cite{Jahn:2018dke} we presented a methodology for computing the topological susceptibility of QCD at temperatures where it is small and standard methods fail. Here we improve on this methodology by removing two barriers…

高能物理 - 格点 · 物理学 2020-02-05 P. Thomas Jahn , Guy D. Moore , Daniel Robaina

The temperature dependence of the topological susceptibility in QCD, chi_t, essentially determines the abundance of the QCD axion in the Universe, and is commonly estimated, based on the instanton picture, to be a certain negative power of…

高能物理 - 唯象学 · 物理学 2015-10-22 Ryuichiro Kitano , Norikazu Yamada

The properties of axions that constitute 100% of cold dark matter (CDM) depend on the tensor-to-scalar ratio $r$ at the end of inflation. If $r=0.20^{+0.07}_{-0.05}$ as reported by the BICEP2 collaboration, then "half" of the CDM axion…

高能物理 - 唯象学 · 物理学 2014-07-09 L. Visinelli , P. Gondolo

If the QCD axion is a significant component of dark matter, and if the universe was once hotter than a few hundred MeV, the axion relic abundance depends on the function $\chi(T)$, the temperature-dependent topological susceptibility.…

高能物理 - 唯象学 · 物理学 2018-02-13 Michael Dine , Patrick Draper , Laurel Stephenson-Haskins , Di Xu

In compact stellar environments, the stability of dense QCD matter requires the simultaneous fulfillment of charge neutrality and beta equilibrium. In this work, we study how temperature and finite chemical potential affect QCD topology and…

高能物理 - 唯象学 · 物理学 2025-12-01 Zhen-Yan Lu , Shu-Peng Wang , Qi Lu , Bo-Nan Zhang , Marco Ruggieri

The QCD axion offers a natural resolution to the strong CP problem and provides a compelling dark matter candidate. If the QCD axion constitutes all the dark matter, the simplest models pick out a narrow range of masses around $100\,\mu{\rm…

高能物理 - 唯象学 · 物理学 2023-10-31 David Cyncynates , Jedidiah O. Thompson

First I will review the QCD theta problem and the Peccei-Quinn solution, with its new particle, the axion. I will review the possibility of the axion as dark matter. If PQ symmetry was restored at some point in the hot early Universe, it…

高能物理 - 唯象学 · 物理学 2018-04-18 Guy D. Moore

One intriguing BSM particle is the QCD axion, which could simultaneously provide a solution to the Strong CP problem and account for some, if not all, of the dark matter density in the universe. This particle is a pNGB of the conjectured…

高能物理 - 唯象学 · 物理学 2015-08-19 Evan Berkowitz , Michael I. Buchoff , Enrico Rinaldi

In an axiverse with numerous axions, the cosmological moduli problem poses a significant challenge because the abundance of axions can easily exceed that of dark matter. The well-established stochastic axion scenario offers a simple…

高能物理 - 唯象学 · 物理学 2023-09-06 Kai Murai , Fuminobu Takahashi , Wen Yin

We introduce a reweighting technique which allows for a continuous sampling of temperatures in a single simulation and employ it to compute the temperature dependence of the QCD topological susceptibility at high temperatures. The method…

高能物理 - 格点 · 物理学 2021-07-14 P. Thomas Jahn , Parikshit M. Junnarkar , Guy D. Moore , Daniel Robaina

We determine the magnetic susceptibility of thermal QCD matter by means of first principles lattice simulations using staggered quarks with physical masses. A novel method is employed that only requires simulations at zero background field,…

高能物理 - 格点 · 物理学 2020-07-29 Gunnar S. Bali , Gergely Endrődi , Stefano Piemonte

We present results on QCD with four dynamical flavors in the temperature range $0.9 \lesssim T/T_c \lesssim 2$. We have performed lattice simulations with Wilson fermions at maximal twist and measured the topological charge with gluonic and…

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