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Cosmology on ultralarge scales with intensity mapping of the neutral hydrogen 21 cm emission: limits on primordial non-Gaussianity.

Abstract:
The large-scale structure of the Universe supplies crucial information about the physical processes at play at early times. Unresolved maps of the intensity of 21 cm emission from neutral hydrogen HI at redshifts z=/~1-5 are the best hope of accessing the ultralarge-scale information, directly related to the early Universe. A purpose-built HI intensity experiment may be used to detect the large scale effects of primordial non-Gaussianity, placing stringent bounds on different models of inflation. We argue that it may be possible to place tight constraints on the non-Gaussianity parameter f(NL), with an error close to σ(f(NL))~1.
Publication status:
Published

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Publisher copy:
10.1103/physrevlett.111.171302

Authors


Journal:
Physical Review Letters More from this journal
Volume:
111
Issue:
17
Pages:
171302
Publication date:
2013-10-01
DOI:
EISSN:
1079-7114
ISSN:
0031-9007


Language:
English
Pubs id:
pubs:439897
UUID:
uuid:69c5dc4a-9ae5-4c5a-9438-03b819e7994d
Local pid:
pubs:439897
Source identifiers:
439897
Deposit date:
2014-05-14
ARK identifier:

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