Theoretical implications of detecting gravitational waves

作者: Ghazal Geshnizjani , William H. Kinney

DOI: 10.1088/1475-7516/2015/08/008

关键词: Cosmological perturbation theoryGeneral relativityAstrophysicsEnergy conditionUniverseClassical mechanicsPhysicsInflation (cosmology)Dark energyMetric expansion of spaceDe Sitter universe

摘要: This paper is the third in a series of theorems which state how cosmological observations can provide evidence for an early phase acceleration universe. Previous demonstrated that observed power spectrum scalar perturbations forces all possible alternative theories inflation to other than General Relativity. It was shown generically, without accelerated expansion, these alternatives have break at least one following tenets classical general relativity: Null Energy Condition (NEC), subluminal signal propagation, or sub-Planckian energy densities. In this we prove detection primordial gravitational waves large scales independent support expansion. proof does not rely on spectral index tensor modes but relies validity quantum field theory curved space time and being sourced from adiabatic vacuum fluctuations. Our approach, like case scalars, by contradiction: investigate possibility detectable fluctuations non-accelerating, universe using perturbation derive contradictory limits dynamics. The contradiction implies more our axioms must been broken. bound only of, also stronger obtained spectrum.

参考文章(31)
A.A. Starobinsky, A new type of isotropic cosmological models without singularity Physics Letters B. ,vol. 91, pp. 99- 102 ,(1980) , 10.1016/0370-2693(80)90670-X
Yi-Fu Cai, Taotao Qiu, Robert Brandenberger, Xinmin Zhang, Nonsingular cosmology with a scale-invariant spectrum of cosmological perturbations from Lee-Wick theory Physical Review D. ,vol. 80, pp. 023511- ,(2009) , 10.1103/PHYSREVD.80.023511
Brian A. Powell, William H. Kinney, Pre-inflationary vacuum in the cosmic microwave background Physical Review D. ,vol. 76, pp. 063512- ,(2007) , 10.1103/PHYSREVD.76.063512
Paolo Creminelli, Jérôme Gleyzes, Jorge Noreña, Filippo Vernizzi, Resilience of the standard predictions for primordial tensor modes Physical Review Letters. ,vol. 113, pp. 231301- ,(2014) , 10.1103/PHYSREVLETT.113.231301
Gregory Walter Horndeski, Conservation of charge and the Einstein–Maxwell field equations Journal of Mathematical Physics. ,vol. 17, pp. 1980- 1987 ,(1976) , 10.1063/1.522837
Adam Moss, Levon Pogosian, Did BICEP2 see vector modes? First B-mode constraints on cosmic defects. Physical Review Letters. ,vol. 112, pp. 171302- ,(2014) , 10.1103/PHYSREVLETT.112.171302
Abhineet Agarwal, Niayesh Afshordi, Thermal Tachyacoustic Cosmology Physical Review D. ,vol. 90, pp. 043528- ,(2014) , 10.1103/PHYSREVD.90.043528
Andreas Albrecht, Paul J. Steinhardt, Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking Physical Review Letters. ,vol. 48, pp. 1220- 1223 ,(1982) , 10.1103/PHYSREVLETT.48.1220