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新一类基于时空测不准原理的幂律暴涨宇宙 被引量:2

A new class of power-law inflation based on space-time uncertainty principle
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摘要 在幂律暴涨宇宙中,以时空测不准原理作为出发点,提出一种新的计算模函数的方法.该方法能够使时空非对易效应以线性的形式贡献到密度扰动的谱指数中.通过分析和比较,发现这一类新的幂律暴涨宇宙模型能够预言一个比较大的张标比,该预言非常好地符合最新的实验观测结果. Based on space-time uncertainty principle, the authors propose a new class of power-law inflation. By using a new method of solving the mode function, a linear term contributes to the spectral index of the power spectra. In this model, it could predict a large tensor-to-scalar ratio, which is well consistent with latest observations.
出处 《上海师范大学学报(自然科学版)》 2014年第4期369-377,共9页 Journal of Shanghai Normal University(Natural Sciences)
基金 国家自然科学基金(11047138) 上海市晨光计划(12CG51) 国家教育基金(2009312711004) 上海市自然科学基金(10ZR1422000)
关键词 暴涨宇宙 时空 测不准原理 张标比 inflation space-time uncertainty principle tensor-to-scalar ratio
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参考文献20

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同被引文献61

  • 1GUTH A H.The inflationary universe:A possible solution to the horizon and flatness problems[J].Phys Rev D,1981,23(347):347-356.
  • 2LINDE A D.A new inflationary universe scenario:A possible solution of the horizon,flatness,homogeneity,isotropy and primordial monopole problems[J].Phys Lett B,1982,108 (6):389-393.
  • 3ALBRECHT A,STEINHARDT P J.Cosmology for grand unified theories with radiatively induced symmetry breaking[J].Phys Rev Lett,1982,48:1220-1223.
  • 4FENG C J,LI X Z.Is non-minimal inflation eternal[J].Nucl Phys B,2010,841 (1-2):178-187.
  • 5FENG C J,LI X Z,SARIDAKIS E N.Preventing eternality in phantom inflation[J].Phys Rev D,2010,82 (2):023526.
  • 6CAI Y F,WANG Y.Noncommutative eternal inflation possible[J].Journal of Cosmology and Astroparticle Physics,2007,06:022,1-10.
  • 7HINSHAW G,LARSON D,KOMATSU E,et al.[WMAP Collaboration].Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:Cosmological parameter results[J].Astrophys J Suppl 2013,208 (2):19.
  • 8ADE P A R,AGHANIM N,ARMITAGE-CAPLAN C,et al.[Planck Collaboration].Planck 2013 results.ⅩⅫ.Constraints on inflation[J/OL].arXiv:1303.5082[astro-ph.C O].
  • 9ADE P A R,AIKIN R W,BARKATS D,et al.[BICEP2 Collaboration].BICEP2 Ⅰ:Detection of B-mode polarization at degree angular scales[J/OL].arXiv:1403.3985[astro-ph.CO].
  • 10ARMENDARIZ-PICON C,DAMOUR T,MUKHANOV V F.K-inflation[J].Phys Lett B,1999,458(2-3):209-218.

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