Evidence for an inflationary phase transition from the LSS and CMB anisotropy data
(2000)
Review of particle physics
15:1-4 (2000) 1-878
Abstract:
This biennial Review summarizes much of Particle Physics. Using data from previous editions, plus 2000 new measurements from 610 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. 漏 2000 Regents of the University of California.On the APM power spectrum and the CMB anisotropy: Evidence for a phase transition during inflation?
(2000)
Thermalisation after inflation
ArXiv hep-ph/0009078 (2000)
Abstract:
During (re)heating of the universe after inflation, the relativistic decay products of the inflaton field $蠁$ must lose energy and additional particles must be produced to attain a thermalised state at a temperature $T_{\reh}$. We estimate the rate of energy loss via elastic and inelastic scattering interactions. Elastic scattering is an inefficient energy loss mechanism so inelastic processes, although higher order in the coupling $伪$, can be faster because more energy is transfered. The timescale to produce a particle number density of ${\cal O}(T_{\reh}^3)$ is the inelastic energy loss timescale, $\sim(伪^3 n_蠁/T_{\reh}^2)^{-1}$.Thermalisation after inflation
(2000)