Large non-Gaussianities in the effective field theory approach to single-field inflation: the bispectrum

被引:60
作者
Bartolo, Nicola [1 ,2 ]
Fasiello, Matteo [3 ,4 ]
Matarrese, Sabino [1 ,2 ]
Riotto, Antonio [1 ,5 ]
机构
[1] Univ Padua, Dipartimento Fis G Galilei, I-35131 Padua, Italy
[2] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy
[3] Univ Milano Bicocca, Dipartimento Fis G Occhialini, I-20126 Milan, Italy
[4] Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy
[5] CERN, Div Theory, CH-1211 Geneva, Switzerland
关键词
inflation; non-gaussianity; cosmological perturbation theory; ONE-LOOP CORRECTIONS; MICROWAVE; PERTURBATIONS;
D O I
10.1088/1475-7516/2010/08/008
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The methods of effective field theory are used to study generic theories of inflation with a single inflaton field and to perform a general analysis of the associated non-Gaussianities. We investigate the amplitudes and shapes of the various generic three-point correlators, the bispectra, which may be generated by different classes of single-field inflationary models. Besides the well-known results for the DBI-like models and the ghost inflationary theories, we point out that curvature-related interactions may give rise to large non-Gaussianities in the form of bispectra characterized by a flat shape which, quite interestingly, is independently produced by several interaction terms. In a subsequent work, we will perform a similar general analysis for the non-Gaussianities generated by the generic four-point correlator, the trispectrum.
引用
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页数:30
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