Possible Explanation to Low CMB Quadrupole
arXiv:astro-ph/0502343 · doi:10.1103/PhysRevD.71.087301
Abstract
The universe might experience many cycles with different vacua. The slow-roll inflation may be preceded by kinetic-dominated contraction occurring in "adjacent" vacua during some cycles. In this report we briefly show this phenomenon may lead to a cutoff of primordial power spectrum. Thus in some sense the CMB at large angular scale might encode the information of other vacua.
10 pages, 3 eps figures, accepted for publication in PRD, v2 revised with published version
References in corpus (8)
- A Low CMB Quadrupole from Dark Energy Isocurvature Perturbations
- A CMB/Dark Energy Cosmic Duality
- Multiple inflation and the WMAP 'glitches'
- A Framework for the Landscape
- Can Universe Experience Many Cycles with Different Vacua ?
- Stochastic Inflation and the Lower Multipoles in the CMB Anisotropies
- Reconstructing the Primordial Spectrum with CMB Temperature and Polarization
- Making waves on CMB power spectrum and inflaton dynamics
Cited by in corpus (72)
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Cosmic Microwave Background Quadrupole and Ellipsoidal Universe
- Ellipsoidal Universe Can Solve The CMB Quadrupole Problem
- The Effective Field Theory of nonsingular cosmology
- Obtaining the CMB anomalies with a bounce from the contracting phase to inflation
- On Perturbations of Quintom Bounce
- CMB multipole measurements in the presence of foregrounds
- A covariant Lagrangian for stable nonsingular bounce
- Observational issues in loop quantum cosmology
- The Effective Field Theory of nonsingular cosmology: II
- A Model of Universe Anisotropization
- CMB Imprints of a Pre-Inflationary Climbing Phase
- CMB quadrupole suppression: I. Initial conditions of inflationary perturbations
- Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
- The CMB Quadrupole depression produced by early fast-roll inflation: MCMC analysis of WMAP and SDSS data
- The pre-inflationary and inflationary fast-roll eras and their signatures in the low CMB multipoles
- A Complete Statistical Analysis for the Quadrupole Amplitude in an Ellipsoidal Universe
- Intermittent null energy condition violations during inflation and primordial gravitational waves
- Anisotropic dark energy and ellipsoidal universe
- The Effective Theory of Inflation in the Standard Model of the Universe and the CMB+LSS data analysis
- CMB anomalies from an inflationary model in string theory
- Pulsar timing array observations as possible hints for nonsingular cosmology
- Pre-inflationary primordial perturbations
- Bounce Inflation Cosmology with Standard Model Higgs Boson
- Pre - Inflationary Clues from String Theory ?
- Cosmic Parallax in Ellipsoidal Universe
- Singular Cosmology Unifying Early and Late-time Acceleration with Matter and Radiation Domination Era
- Patterns of galaxy spin directions in SDSS and Pan-STARRS show parity violation and multipoles
- Pre-inflation and Trans-Planckian Censorship
- Gauss-Bonnet Cosmology Unifying Late and Early-time Acceleration Eras with Intermediate Eras
- Primordial perturbations with pre-inflationary bounce
- Slow-Roll Inflation Preceded by a Topological Defect Phase à la Chaplygin Gas
- On the Viability of the Intermediate Inflation Scenario with Gravity
- Bounce in GR and higher-order derivative operators
- Observational hints on the Big Bounce
- Smoking guns of a bounce in modified theories of gravity through the spectrum of the gravitational waves
- Generating enhanced primordial GWs during inflation with intermittent violation of NEC and diminishment of GW propagating speed
- Magnetogenesis in bouncing cosmology
- Amplification of Curvature Perturbations in Cyclic Cosmology
- Pre-inflationary genesis with CMB B-mode polarization
- Implication of GW170817 for cosmological bounces
- Brane SUSY Breaking and the Gravitino Mass
- A Multiple Step-like Spectrum of Primordial Perturbation
- Parity violation in pre-inflationary bounce
- Phantom Inflation with A Steplike Potential
- Perturbative unitarity and NEC violation in genesis cosmology
- Can the Big Bang Singularity be avoided by a single scalar field?
- Perturbations of bounce inflation scenario from modified gravity revisited
- Smooth coarse-graining and colored noise dynamics in stochastic inflation
- The interacting multiverse and its effect on the cosmic microwave background
- Scalar Perturbations Through Cycles
- Implication of island for inflation and primordial perturbations
- Analysis of spin directions of galaxies in the DESI Legacy Survey
- New evidence and analysis of cosmological-scale asymmetry in galaxy spin directions
- Density fluctuations in -deformed inflationary universe
- Analysis of spiral galaxies from four telescopes shows large-scale patterns of asymmetry in galaxy spin directions
- Towards the bounce inflationary gravitational wave
- Pre-inflation from the multiverse: Can it solve the quadrupole problem in the cosmic microwave background?
- Large-scale asymmetry in the distribution of galaxy spin directions -- analysis and reproduction
- Large-scale asymmetry in galaxy spin directions -- analysis of galaxies with spectra in DES, SDSS, and DESI Legacy Survey
- Thermal gravitational-wave background in the general pre-inflationary scenario
- Type IV singular bouncing cosmology from Gravity
- Parity-violating primordial gravitational waves from null energy condition violation
- Signature of short distance physics on inflation power spectrum and CMB anisotropy
- Large-scale patterns of galaxy spin rotation show cosmological-scale parity violation and multipoles
- Cosmological evolutions of nonlinear massive gravity
- Low- CMB from String-Scale SUSY Breaking?
- A Model of Large Quintessence Isocurvature Fluctuations and Low CMB Quadrupole
- An Inflationary Scenario Taking into Account of Possible Dark Energy Effects in the Early Universe
- AdS cycles in eternally inflating background
- Multipole alignment in the large-scale distribution of spin direction of spiral galaxies
- Nonlinear Spinor Fields in LRS Bianchi type-I spacetime: Theory and observation