Imperial College London

Prof Joao Magueijo

Faculty of Natural SciencesDepartment of Physics

Professor of Physics
 
 
 
//

Contact

 

j.magueijo Website

 
 
//

Location

 

Huxley BuildingSouth Kensington Campus

//

Summary

 

Publications

Citation

BibTex format

@article{Magueijo:2017:11/014,
author = {Magueijo, J},
doi = {11/014},
journal = {Journal of Cosmology and Astroparticle Physics},
title = {The phenomenology of squeezing and its status in non-inflationary theories},
url = {http://dx.doi.org/10.1088/1475-7516/2017/11/014},
volume = {2017},
year = {2017}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - In this paper we skim the true phenomenological requirements behind the concept of inflationary squeezing. We argue that all that is required is that at horizon re-entry the fluctuations form standing waves with the correct temporal phase (specifically, sine waves). We quantify this requirement and relate it to the initial conditions fed into the radiation dominated epoch by whatever phase of the Universe produced the fluctuations. The only relevant quantity turns out to be the degree of suppression of the momentum, p, of the fluctuations, y, which we measure by σ~ ω2 |y|2/|p|2. Even though σ equals the squeezing parameter, s, in the case of inflation and bimetric varying speed of light scenarios, this is not true in general, specifically in some bouncing Universe models. It is also not necessary to produce a large σ at the end of the primordial phase: it is enough that σ be not too small. This is the case with scenarios based on modified dispersion relations (MDR) emulating the dispersion relations of Horava-Lifshitz theory, which produce σ~ 1, enough to comply with the observational requirements. Scenarios based on MDR leading to a slightly red spectrum are also examined, and shown to satisfy the observational constraints.
AU - Magueijo,J
DO - 11/014
PY - 2017///
SN - 1475-7516
TI - The phenomenology of squeezing and its status in non-inflationary theories
T2 - Journal of Cosmology and Astroparticle Physics
UR - http://dx.doi.org/10.1088/1475-7516/2017/11/014
UR - http://hdl.handle.net/10044/1/54404
VL - 2017
ER -