2009/08/31 by Olivier Wantz, E. P. S. Shellard · 2 citations
Physics and Astronomy · #Axion #Combinatorics #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Grand canonical ensemble #Instanton #Lambda #Mathematical physics #Monte Carlo method #Particle physics #Particle physics theoretical and experimental studies #Phase transition #Physics #Quantum mechanics #Quark #Topology (electrical circuits) #astro-ph.CO #hep-lat #hep-ph
paper · pdf · doi:10.1016/j.nuclphysb.2009.12.005
published as Nucl.Phys.B829:110-160,2010 · 65 pages, 36 figures. As accepted by Nucl.Phys.B
openalex publication_date 2009/12/15 · arxiv created 2010/01/14 · arxiv updated 2010/02/08 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
This is the last in a series of papers on the topological susceptibility in the interacting instanton liquid model (IILM). We will derive improved finite temperature interactions to study the thermodynamic limit of grand canonical Monte Carlo simulations in the quenched and unquenched case with light, physical quark masses. In particular, we will be interested in chiral symmetry breaking. The paper culminates by giving, for the first time, a well-motivated temperature-dependent axion mass. Especially, this work finally provides a computation of the axion mass in the low temperature regime, m2a f2a = 1.46 10-3Λ4 \frac1+0.50 T/Λ1+(3.53 T/Λ)7.48. It connects smoothly to the high temperature dilute gas approximation; the latter is improved by including quark threshold effects. To compare with earlier studies, we also provide the usual power-law m2a = (αa Λ4)/(fa2 (T/Λ)n), where Λ=400\unitsMeV, n=6.68 and α=1.68 10-7.