Prospects for Cosmological Collider Physics
Oct 20, 2016
19 pages
Published in:
- JCAP 03 (2017) 050
- Published: Mar 27, 2017
e-Print:
- 1610.06559 [astro-ph.CO]
View in:
Citations per year
Abstract: (IOP)
It is generally expected that heavy fields are present during inflation, which can leave their imprint in late-time cosmological observables. The main signature of these fields is a small amount of distinctly shaped non-Gaussianity, which if detected, would provide a wealth of information about the particle spectrum of the inflationary Universe. Here we investigate to what extent these signatures can be detected or constrained using futuristic 21-cm surveys. We construct model-independent templates that extract the squeezed-limit behavior of the bispectrum, and examine their overlap with standard inflationary shapes and secondary non-Gaussianities. We then use these templates to forecast detection thresholds for different masses and couplings using a 3D reconstruction of modes during the dark ages (z~ 30–100). We consider interactions of several broad classes of models and quantify their detectability as a function of the baseline of a dark ages interferometer. Our analysis shows that there exists the tantalizing possibility of discovering new particles with different masses and interactions with future 21-cm surveys.Note:
- 19 pages, 12 figures, minor improvements, references, typos
- particle: spectrum
- inflation: model
- non-Gaussianity
- cosmological model
- fluctuation: primordial
- statistical analysis
- interferometer
- new particle
- bispectrum
References(63)
Figures(16)
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