Inflation from quantum geometry

被引:161
作者
Bojowald, M [1 ]
机构
[1] Penn State Univ, Ctr Gravitat Phys & Geometry, Davey Lab 104, University Pk, PA 16802 USA
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevLett.89.261301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Quantum geometry predicts that a universe evolves through an inflationary phase at small volume before exiting gracefully into a standard Friedmann phase. This does not require the introduction of additional matter fields with ad hoc potentials; rather, it occurs because of a quantum gravity modification of the kinetic part of ordinary matter Hamiltonians. An application of the same mechanism can explain why the present day cosmological acceleration is so tiny.
引用
收藏
页数:4
相关论文
共 23 条
  • [1] ALEXANDER S, HEPTH0108190
  • [2] [Anonymous], GRQC0110034
  • [3] Quantum geometry and black hole entropy
    Ashtekar, A
    Baez, J
    Corichi, A
    Krasnov, K
    [J]. PHYSICAL REVIEW LETTERS, 1998, 80 (05) : 904 - 907
  • [4] ASHTEKAR A, 2001, ADV THEOR MATH PHYS, V4, P1
  • [5] Ashtekar Abhay., 1991, LECT NONPERTURBATIVE
  • [6] Isotropic loop quantum cosmology with matter
    Bojowald, M
    Hinterleitner, F
    [J]. PHYSICAL REVIEW D, 2002, 66 (10):
  • [7] Isotropic loop quantum cosmology
    Bojowald, M
    [J]. CLASSICAL AND QUANTUM GRAVITY, 2002, 19 (10) : 2717 - 2741
  • [8] Dynamical initial conditions in quantum cosmology
    Bojowald, M
    [J]. PHYSICAL REVIEW LETTERS, 2001, 87 (12) : 1 - 121301
  • [9] Quantization ambiguities in isotropic quantum geometry
    Bojowald, M
    [J]. CLASSICAL AND QUANTUM GRAVITY, 2002, 19 (20) : 5113 - 5129
  • [10] The semiclassical limit of loop quantum cosmology
    Bojowald, M
    [J]. CLASSICAL AND QUANTUM GRAVITY, 2001, 18 (18) : L109 - L116