### 摘要

We consider two different definitions for loop corrections to the primordial power spectra. One of these is to simply correct the mode functions in the tree order relations using the linearized effective field equations. The second definition involves the spatial Fourier transform of the two-point correlator. Although the two definitions agree at tree order, we show that they disagree at one loop using the Schwinger-Keldysh formalism, so there are at least two plausible ways of loop correcting the tree order result. We discuss the advantages and disadvantages of each.

原文 | English |
---|---|

文章編號 | 064053 |

期刊 | Physical Review D - Particles, Fields, Gravitation and Cosmology |

卷 | 89 |

發行號 | 6 |

DOIs | |

出版狀態 | Published - 2014 三月 24 |

### 指紋

### All Science Journal Classification (ASJC) codes

- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)

### 引用此文

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**Alternate definitions of loop corrections to the primordial power spectra.** / Miao, Shun-Pei; Park, Sohyun.

研究成果: Article

TY - JOUR

T1 - Alternate definitions of loop corrections to the primordial power spectra

AU - Miao, Shun-Pei

AU - Park, Sohyun

PY - 2014/3/24

Y1 - 2014/3/24

N2 - We consider two different definitions for loop corrections to the primordial power spectra. One of these is to simply correct the mode functions in the tree order relations using the linearized effective field equations. The second definition involves the spatial Fourier transform of the two-point correlator. Although the two definitions agree at tree order, we show that they disagree at one loop using the Schwinger-Keldysh formalism, so there are at least two plausible ways of loop correcting the tree order result. We discuss the advantages and disadvantages of each.

AB - We consider two different definitions for loop corrections to the primordial power spectra. One of these is to simply correct the mode functions in the tree order relations using the linearized effective field equations. The second definition involves the spatial Fourier transform of the two-point correlator. Although the two definitions agree at tree order, we show that they disagree at one loop using the Schwinger-Keldysh formalism, so there are at least two plausible ways of loop correcting the tree order result. We discuss the advantages and disadvantages of each.

UR - http://www.scopus.com/inward/record.url?scp=84898725333&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84898725333&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.89.064053

DO - 10.1103/PhysRevD.89.064053

M3 - Article

AN - SCOPUS:84898725333

VL - 89

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

SN - 1550-7998

IS - 6

M1 - 064053

ER -