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Implications of purely classical gravity for inflationary tensor modes

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Implications of purely classical gravity for inflationary tensor modes. / Ashoorioon, Amjad; S. Bhupal Dev, P.; Mazumdar, Anupam.
In: arxiv.org, 20.11.2012.

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@article{0a95160bd0134e699c8d984e5d7cdb4b,
title = "Implications of purely classical gravity for inflationary tensor modes",
abstract = "We discuss the implications of purely classical, instead of quantum, theory of gravity for the gravitational wave spectrum generated during inflation. We show that a positive detection of primordial gravitational waves will no longer suffice to determine the scale of inflation in this case -- even a high-scale model of inflation can bypass the observational constraints due to large uncertainties in the initial classical amplitude of the tensor modes.",
keywords = "hep-th, astro-ph.CO, gr-qc, hep-ph",
author = "Amjad Ashoorioon and {S. Bhupal Dev}, P. and Anupam Mazumdar",
note = "v1: 4 pages; v2:6 pages. This is the first paper to argue that a positive detection of B-modes would signify that initial conditions for primordial gravity waves is set by quantum initial conditions and not by classical ones",
year = "2012",
month = nov,
day = "20",
language = "English",
journal = "arxiv.org",

}

RIS

TY - JOUR

T1 - Implications of purely classical gravity for inflationary tensor modes

AU - Ashoorioon, Amjad

AU - S. Bhupal Dev, P.

AU - Mazumdar, Anupam

N1 - v1: 4 pages; v2:6 pages. This is the first paper to argue that a positive detection of B-modes would signify that initial conditions for primordial gravity waves is set by quantum initial conditions and not by classical ones

PY - 2012/11/20

Y1 - 2012/11/20

N2 - We discuss the implications of purely classical, instead of quantum, theory of gravity for the gravitational wave spectrum generated during inflation. We show that a positive detection of primordial gravitational waves will no longer suffice to determine the scale of inflation in this case -- even a high-scale model of inflation can bypass the observational constraints due to large uncertainties in the initial classical amplitude of the tensor modes.

AB - We discuss the implications of purely classical, instead of quantum, theory of gravity for the gravitational wave spectrum generated during inflation. We show that a positive detection of primordial gravitational waves will no longer suffice to determine the scale of inflation in this case -- even a high-scale model of inflation can bypass the observational constraints due to large uncertainties in the initial classical amplitude of the tensor modes.

KW - hep-th

KW - astro-ph.CO

KW - gr-qc

KW - hep-ph

M3 - Journal article

JO - arxiv.org

JF - arxiv.org

ER -