| 000 | 03479nam a22005417a 4500 | ||
|---|---|---|---|
| 001 | sulb-eb0025914 | ||
| 003 | BD-SySUS | ||
| 005 | 20160413122554.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 130710s2013 ja | s |||| 0|eng d | ||
| 020 |
_a9784431541806 _9978-4-431-54180-6 |
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| 024 | 7 |
_a10.1007/978-4-431-54180-6 _2doi |
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| 050 | 4 | _aQB1-991 | |
| 050 | 4 | _aQB460-466 | |
| 050 | 4 | _aQB980-991 | |
| 072 | 7 |
_aPGC _2bicssc |
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| 072 | 7 |
_aSCI004000 _2bisacsh |
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| 072 | 7 |
_aSCI005000 _2bisacsh |
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| 082 | 0 | 4 |
_a520 _223 |
| 100 | 1 |
_aShiraishi, Maresuke. _eauthor. |
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| 245 | 1 | 0 |
_aProbing the Early Universe with the CMB Scalar, Vector and Tensor Bispectrum _h[electronic resource] / _cby Maresuke Shiraishi. |
| 264 | 1 |
_aTokyo : _bSpringer Japan : _bImprint: Springer, _c2013. |
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| 300 |
_aXIII, 180 p. _bonline resource. |
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| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
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| 338 |
_aonline resource _bcr _2rdacarrier |
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| 347 |
_atext file _bPDF _2rda |
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| 490 | 1 |
_aSpringer Theses, Recognizing Outstanding Ph.D. Research, _x2190-5053 |
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| 505 | 0 | _aIntroduction -- Fluctuations in the inflation -- Fluctuations in cosmic microwave background radiation -- Primordial non-Gaussianities -- General formalism for the CMB bispectrum from primordial scalar, vector and tensor non-Gaussianities -- CMB bispectrum Induced by the two scalars and a graviton correlator -- Violation of the rotational invariance in the CMB bispectrum -- Parity violation of gravitons in the CMB bispectrum -- CMB bispectrum generated from primordial magnetic fields -- Conclusion. | |
| 520 | _aThe non-Gaussianity in the primordial density fluctuations is a key feature to clarify the early Universe and it has been probed with the Cosmic Microwave Background (CMB) bispectrum. In recent years, we have treated the novel-type CMB bispectra, which originate from the vector- and tensor-mode perturbations and include the violation of the rotational or parity invariance. On the basis of our current works, this thesis provides the general formalism for the CMB bispectrum sourced by the non-Gaussianity in the scalar, vector and tensor-mode perturbations. Applying this formalism, we calculate the CMB bispectra from the two scalars and a graviton correlation and primordial magnetic fields, and then outline new constraints on these magnitudes. Furthermore, this formalism can be easily extended to the cases where the rotational or parity invariance is broken. We also compute the CMB bispectra from the scalar-mode non-Gaussianities with a preferred direction and the tensor-mode non-Gaussianities induced by the parity-violating Weyl cubic terms. Here, we show that these bispectra include unique signals, which any symmetry-invariant models can never produce. | ||
| 650 | 0 | _aPhysics. | |
| 650 | 0 | _aMathematical physics. | |
| 650 | 0 | _aAstronomy. | |
| 650 | 0 | _aAstrophysics. | |
| 650 | 0 | _aCosmology. | |
| 650 | 1 | 4 | _aPhysics. |
| 650 | 2 | 4 | _aAstronomy, Astrophysics and Cosmology. |
| 650 | 2 | 4 | _aMathematical Methods in Physics. |
| 650 | 2 | 4 | _aMathematical Physics. |
| 710 | 2 | _aSpringerLink (Online service) | |
| 773 | 0 | _tSpringer eBooks | |
| 776 | 0 | 8 |
_iPrinted edition: _z9784431541790 |
| 830 | 0 |
_aSpringer Theses, Recognizing Outstanding Ph.D. Research, _x2190-5053 |
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| 856 | 4 | 0 | _uhttp://dx.doi.org/10.1007/978-4-431-54180-6 |
| 912 | _aZDB-2-PHA | ||
| 942 |
_2Dewey Decimal Classification _ceBooks |
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| 999 |
_c48006 _d48006 |
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