Anomalous cosmic-microwave-background polarization and gravitational chirality

被引:88
作者
Contaldi, Carlo R. [1 ]
Magueijo, Joao [1 ]
Smolin, Lee [2 ]
机构
[1] Univ London Imperial Coll Sci Technol & Med, London SW7 2BZ, England
[2] Perimeter Inst, Waterloo, ON N2L 2Y5, Canada
基金
英国科学技术设施理事会;
关键词
D O I
10.1103/PhysRevLett.101.141101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We consider the possibility that gravity breaks parity, with left and right-handed gravitons coupling to matter with a different Newton's constant and show that this would affect their zero-point vacuum fluctuations during inflation. Should there be a cosmic background of gravity waves, the effect would translate into anomalous cosmic microwave background polarization. Nonvanishing temperature-magnetic (TB) mode [and electric-magnetic mode] components emerge, revealing interesting experimental targets. Indeed, if reasonable chirality is present a TB measurement would provide the easiest way to detect a gravitational wave background. We speculate on the theoretical implications of such an observation.
引用
收藏
页数:4
相关论文
共 29 条
  • [1] ALEXANDER S, ARXIV07064481
  • [2] Leptogenesis from gravity waves in models of inflation
    Alexander, SHS
    Peskin, ME
    Sheikh-Jabbari, MM
    [J]. PHYSICAL REVIEW LETTERS, 2006, 96 (08) : 1 - 4
  • [3] BOND JR, 1984, ASTROPHYS J, V285, pL45, DOI 10.1086/184362
  • [4] CHALLINOR A, ARXIVASTROPH0403344
  • [5] CHALLINOR A, ARXIVASTROPH0502093
  • [6] CONTALDI CR, IN PRESS
  • [7] Leptogenesis from pseudo-scalar driven inflation
    Fischler, Willy
    Paban, Sonia
    [J]. JOURNAL OF HIGH ENERGY PHYSICS, 2007, (10):
  • [8] Quantum gravity, torsion, parity violation, and all that
    Freidel, L
    Minic, D
    Takeuchi, T
    [J]. PHYSICAL REVIEW D, 2005, 72 (10):
  • [9] Statistics of cosmic microwave background polarization
    Kamionkowski, M
    Kosowsky, A
    Stebbins, A
    [J]. PHYSICAL REVIEW D, 1997, 55 (12): : 7368 - 7388
  • [10] LORENTZ INVARIANCE AND GRAVITATIONAL FIELD
    KIBBLE, TW
    [J]. JOURNAL OF MATHEMATICAL PHYSICS, 1961, 2 (02) : 212 - &