Miniclusters in the axiverse
From MaRDI portal
Publication:1692804
DOI10.1007/JHEP02(2017)046zbMath1377.83156arXiv1609.00208OpenAlexW2512129694MaRDI QIDQ1692804
Publication date: 10 January 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1609.00208
Related Items (4)
A self-consistent wave description of axion miniclusters and their survival in the galaxy ⋮ Global cosmic string networks as a function of tension ⋮ New scenario of QCD axion clump formation. Part I. Linear analysis ⋮ Can axion clumps be formed in a pre-inflationary scenario?
Cites Work
- Universal mechanism of (semi-classical) deconfinement and \(\theta\)-dependence for all simple groups
- An \(M\) theory solution to the strong CP-problem, and constraints on the axiverse
- \(\theta \) dependence of \(SU(N)\) gauge theories
- \(\mathrm{SU}(N)\) gauge theories at large \(N\)
- Topology of \(\text{SU}(N)\) gauge theories at \(T \simeq 0\) and \(T \simeq T_{c}\)
- The deconfining phase transition in SU(N\(_c\)) gauge theories
- Free energy and \(\theta\) dependence of SU(N) gauge theories
- The type IIB string axiverse and its low-energy phenomenology
- Notes on theta dependence in holographic Yang-Mills
- On axionic dark matter in Type IIA string theory
This page was built for publication: Miniclusters in the axiverse
