Teststringtheorywithprimordialgravitationalwave.ppt

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1、Low-energy effective string theory in primordial gravitational wave,朴云松University of CAS,USTC-ICTS,2015.4.23,一、动机二、我们的工作三、讨论,Based on 1501.06345, PRD, with Yong Cai and Yu-Tong Wang,The paradigm of early universe: inflation (alternatives ?),Planck 2015 results,As a laboratory,inflation sub-Planck sc

2、ale,LHC,?,1、Primordial scalar perturbation Planck限制, 原初的 “污染”源多2、Primordial gravitational wave 目前只有上限, 没有原初的“污染”源,inflationary lab,string theory,primordial gravitational wave can be non-trivial?,inflationary gravitational wave,BICEP2/Keck and Planck 2015,the low-energy effective action of heterotic

3、string is Metsaev,Tseytlin, Nucl.Phys.B293, 385 (1987),一个例子:,二、我们的工作,The primordial GW,The effect is negligible, if and,Beyond GR,the effective Planck scalethe propagating speed,The change of speed,The change of speed may be non-trivial.,Gasperini,Veneziano 2002,The effect of non-trivial change of s

4、peed,The equation is,the mode is in Bunch-Davis state,Initially,this sets,Inflation background,The perturbation is ,and are determined by the matching conditions.,Inflation background,The result of primordial GWs,is that of slow-roll inflation,The character scale,Detail of the GWs,However, the oscil

5、lation appear for,is inflationary-like,The oscillation can be attributed to other mechanism?,1、 is oscillating, hardly implemented. 2、The production of particles, only a bump-like behavior.,Gary Shiu et.al 1405.0346,Transfer to B-mode polarization spectrum,l=2,65,is the optical depth,三、Discussion,Th

6、e assumptions: 1、Inflation is the paradigm of early universe. 2、The higher-order derivative terms in superstring theory is significant. alter The conclusion: The oscillating GWs is imprinted in CMB B-mode polarization. Hope r0.01.,The physics of oscillation,The low-energy effective action of superstring alters the initial state of mode The Bunch-Davis state only for mode but for mode Note: initial state is not altered by,r =0.05+lense By Yu-Tong Wang,The outlook:,Tegmark, ApJ 464, L35 1996,WMAP 3-year 2006,Planck 2015,The history of CMB TT spectrum observations,Thank You !,

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