{ "id": "1107.0682", "version": "v3", "published": "2011-07-04T17:17:55.000Z", "updated": "2011-11-22T07:33:47.000Z", "title": "Violation of the Rotational Invariance in the CMB Bispectrum", "authors": [ "Maresuke Shiraishi", "Shuichiro Yokoyama" ], "comment": "13 pages, 2 figures. Accepted for publication in PTP", "journal": "Prog. Theor. Phys. 126 (2011), 923-935", "doi": "10.1143/PTP.126.923", "categories": [ "astro-ph.CO", "gr-qc", "hep-ph", "hep-th" ], "abstract": "We investigate a statistical anisotropy on the Cosmic Microwave Background (CMB) bispectrum, which can be generated from the primordial non-Gaussianity induced by quantum fluctuations of a vector field. We find new configurations in the multipole space of the CMB bispectrum given by $\\ell_1 = \\ell_2 + \\ell_3 + 2, |\\ell_2 - \\ell_3| - 2$ and their permutations, which violate the rotational invariance, such as an off-diagonal configuration in the CMB power spectrum. We also find that in a model presented by Yokoyama and Soda (2008), the amplitude of the statistically anisotropic bispectrum in the above configurations becomes as large as that in other configurations such as $\\ell_1 = \\ell_2 + \\ell_3$. As a result, it might be possible to detect these contributions in future experiments, which would give us novel information about the physics of the early Universe.", "revisions": [ { "version": "v3", "updated": "2011-11-22T07:33:47.000Z" } ], "analyses": { "keywords": [ "cmb bispectrum", "rotational invariance", "cosmic microwave background", "cmb power spectrum", "quantum fluctuations" ], "tags": [ "journal article" ], "publication": { "journal": "Progress of Theoretical Physics", "year": 2011, "month": "Nov", "volume": 126, "number": 5, "pages": 923 }, "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable", "inspire": 916784, "adsabs": "2011PThPh.126..923S" } } }