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相关论文: Gravitational Fluctuations as an Alternative to In…

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Power spectra play an important role in the theory of inflation, and their ability to reproduce current observational data to high accuracy is often considered a triumph of inflation, largely because of a lack of credible alternatives. In…

宇宙学与河外天体物理 · 物理学 2020-05-21 Herbert W. Hamber , Lu Heng Sunny Yu , Hasitha E. Pituwala Kankanamge

The ability to reproduce the observed matter power spectrum $P(k)$ to high accuracy is often considered as a triumph of inflation. In this work, we explore an alternative explanation for the power spectrum based on nonperturbative quantum…

广义相对论与量子宇宙学 · 物理学 2019-03-18 Herbert W. Hamber , Lu Heng Sunny Yu

The observed power spectrum of the cosmic microwave background (CMB) is consistent with inflationary cosmology, which predicts a nearly scale-invariant power spectrum of quantum fluctuations of the inflaton field as they exit the Hubble…

高能物理 - 理论 · 物理学 2007-05-23 Leonard Parker

We derive the primordial power spectrum of density fluctuations in the framework of quantum cosmology. For this purpose we perform a Born-Oppenheimer approximation to the Wheeler-DeWitt equation for an inflationary universe with a scalar…

广义相对论与量子宇宙学 · 物理学 2012-01-17 Claus Kiefer , Manuel Kraemer

Noncommutative geometry can provide effective description of physics at very short distances taking into account generic effects of quantum gravity. Inflation amplifies tiny quantum fluctuations in the early universe to macroscopic scales…

宇宙学与河外天体物理 · 物理学 2011-03-18 Tomi S. Koivisto , David F. Mota

Recent measurements of temperature fluctuations in the cosmic microwave background (CMB) indicate that the Universe is flat and that large-scale structure grew via gravitational infall from primordial adiabatic perturbations. Both of these…

天体物理学 · 物理学 2009-10-31 Marc Kamionkowski , Andrew H. Jaffe

Measurements of CMB temperature fluctuations by the Wilkinson Microwave Anisotropy Probe (WMAP) indicate that the fluctuation amplitude in one half of the sky differs from the amplitude in the other half. We show that such an asymmetry…

天体物理学 · 物理学 2008-12-30 Adrienne L. Erickcek , Marc Kamionkowski , Sean M. Carroll

String/M theory inspires an uncertainty relation between space and time which deviates from general relativity. It is possible to explore this deviation from cosmological observations, in particular from the CMB fluctuation spectrum. This…

天体物理学 · 物理学 2008-11-26 Qing-Guo Huang , Miao Li

One of the great triumphs of the inflationary model is the prediction of the flat power spectrum of the CMB fluctuation. The prediction is based on the assumption of the de-Sitter vacuum in the past infinity. However, the true past infinity…

广义相对论与量子宇宙学 · 物理学 2019-03-27 Tadashi Sasaki , Hisao Suzuki

Very recent CMB data of WMAP offers an opportunity to test inflation models, in particular, the running of spectral index is quite new and can be used to rule out some models. We show that an noncommutative spacetime inflation model gives a…

高能物理 - 理论 · 物理学 2009-11-10 Qing Guo Huang , Miao Li

Predictions of the CMB spectrum from a bimetric gravity theory (gr-qc/0101126) are presented. The initial inflationary period in BGT is driven by a vanishingly small speed of gravitational waves v_g in the very early universe. This initial…

天体物理学 · 物理学 2009-11-07 M. A. Clayton , J. W. Moffat

Recent Planck data show the anomalies of CMB fluctuations on large angular scales, which confirms the early observations by WMAP. We continue studying an inflationary model, in which before the slow roll inflation the universe is in a…

宇宙学与河外天体物理 · 物理学 2013-10-15 Zhi-Guo Liu , Zong-Kuan Guo , Yun-Song Piao

We study the inflation process of universe based on the renormalizable quantum gravity formulated as a conformal field theory (CFT). We show that the power-law CFT spectrum approaches to that of the Harrison-Zel'dovich-Peebles type as the…

宇宙学与河外天体物理 · 物理学 2010-05-18 Ken-ji Hamada , Shinichi Horata , Tetsuyuki Yukawa

In this article we review the theory of cosmological inflation with a particular focus on the beautiful connection it provides between the physics of the very small and observations of the very large. We explain how quantum mechanical…

天体物理学 · 物理学 2010-04-30 Daniel Baumann , Hiranya V. Peiris

Inflation provides a unified paradigm for understanding the isotropy of the cosmic microwave background (CMB), the flatness problem, and the origin of large-scale structure. Although the physics responsible for inflation is not yet well…

天体物理学 · 物理学 2015-06-24 Marc Kamionkowski

We show that there are inflationary models for which perturbations in the energy momentum tensor, which are of second order in the scalar field, cannot be neglected. We first specify the conditions under which the usual first order…

天体物理学 · 物理学 2009-10-22 R. Durrer , M. Sakellariadou

The spectrum of the gravitational wave background originating from quantum fluctuations during inflation is calculated numerically for various inflation models over a wide range of frequencies. We take into account four ingredients : the…

天体物理学 · 物理学 2009-05-04 Sachiko Kuroyanagi , Takeshi Chiba , Naoshi Sugiyama

We show that in theories with a nontrivial kinetic term the contribution of the gravitational waves to the CMB fluctuations can be substantially larger than that is naively expected in simple inflationary models. This increase of the…

天体物理学 · 物理学 2014-10-13 V. Mukhanov , A. Vikman

Inflation predicts a stochastic background of gravitational waves over a broad range of frequencies, from those accessible with cosmic microwave background (CMB) measurements, to those accessible directly with gravitational-wave detectors,…

天体物理学 · 物理学 2008-11-26 Tristan L. Smith , Marc Kamionkowski , Asantha Cooray

It is well known that in manifestly Lorentz invariant theories with nontrivial kinetic terms, perturbations around some classical backgrounds can travel faster than light. These exotic "supersonic" models may have interesting consequences…

天体物理学 · 物理学 2009-09-29 Alexander Vikman
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