Higher order corrections to asymptotic-de Sitter inflation

作     者：M.Mohsenzadeh E.Yusofi 

作者机构：Department of PhysicsQom BranchIslamic Azad UniversityQomIran Department of PhysicsAyatollah Amoli BranchIslamic Azad UniversityAmolMazandaranIrana School of AstronomyInstitute for Research in Fundamental Sciences(IPM)P.O.Box 19395-5531TehranIran 

出 版 物：《Chinese Physics C》 (中国物理C（英文版）)

年 卷 期：2017年第41卷第8期

页      面：112-117页

核心收录：

学科分类：02[经济学] 0202[经济学-应用经济学] 0201[经济学-理论经济学] 020204[经济学-金融学（含∶保险学）] 020203[经济学-财政学（含∶税收学）] 020101[经济学-政治经济学] 

基　　金：supported by the Islamic Azad University Qom Branch Qom Iran 

主　　题：initial state trans-Planckian effects inflation 

摘      要：Since trans-Planckian considerations can be associated with the re-definition of the initial vacuum, we investigate further the influence of trans-Planckian physics on the spectra produced by the initial quasi-de Sitter（d S） state during inflation. We use the asymptotic-d S mode to study the trans-Planckian correction of the power spectrum to the quasi-d S inflation. The obtained spectra consist of higher order corrections associated with the type of geometry and harmonic terms sensitive to the fluctuations of space-time（or gravitational waves） during *** an important result, the amplitude of the power spectrum is dependent on the choice of c, i.e. the type of spacetime in the period of inflation. Also, the results are always valid for any asymptotic d S space-time and particularly coincide with the conventional results for d S and flat space-time.