Cited by 116Cosmology and Gravitation TheoriesPulsars and Gravitational Waves ResearchNoncommutative and Quantum Gravity Theories

Spikes in the relic graviton background from quintessential inflation

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Giovannini, Massimo·1999·Classical and Quantum Gravity

Abstract

The energy spectra of gravitational waves (GWs) produced in quintessential inflationary models increase in frequency and exhibit a sharp spike around 170 GHz where the associated fraction of critical energy density presently stored in relic gravitons is of the order of 10 -6 . The maximal energy density present (today) in the stochastic GW background of quintessential origin is mainly constrained by the consistency with the (homogeneous and isotropic) big-bang nucleosynthesis scenario. We contrast our findings with the spectra of ordinary inflationary models and we comment on possible detection strategies for the spike.

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Crossref · 10.1088/0264-9381/16/9/308

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  • In many scenarios with a stiff or ekpyrotic phase, the background dynamics can enhance high-frequency stochastic gravitational waves and tilt the tensor spectrum blue.

    “Third, in many scenarios with a stiff or ekpyrotic phase, the background dynamics can enhance highfrequency stochastic gravitational waves and tilt the tensor spectrum blue [40].”

    From Dynamical systems analysis of an Einstein–Cartan ekpyrotic nonsingular bounce cosmology (2026) · cites this paper as [40]

    The discussion on p. 2 says that a post-inflationary stiff phase produces relic-graviton spectra that are blue and increase with frequency; the conclusion on p. 8 says the resulting signal can be much larger than after a direct transition to radiation domination. The paper addresses quintessential inflation with a stiff phase, but our copy does not address ekpyrotic phases or establish the claim across many scenarios. (LLM, conf=0.87)

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Research works printed but not linked: 5

  1. [3][3] P. J. E. Peebles and A. Vilenkin, Quintessential Inflation , astro-ph/9810509. - · arXiv
  2. [5][5] S. Perlmutter et al., Nature 391 , 51 (1998); A. G. Riess et al., astro-ph/9805201; P. M. Garnavich et al., astro-ph/9806396. - · arXiv
  3. [10][10] M. Giovannini, TUPT-01-99, astro-ph/9903004. - · arXiv
  4. [17][17] B. Allen, in Proceedings of the Les Houches School on Astrophysical Sources of Gravitational Waves, edited by J. Marck and J.P. Lasota (Cambridge University Press, Cambridge England, 1996); B. Allen and J. Romano, Detecting a stochastic background of gravitational radiation: signal processing strategies and sensitivities , WISC-MILW-97TH-14, gr-qc/9710117. - · arXiv
  5. [20][20] K. S. Thorne, in 300 Years of Gravitation ,edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987).

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Authors
Giovannini, M.
Venue
Classical and Quantum Gravity
Published
1999-08-06
Volume
16
Issue
9
Pages
2905-2913
ISSN
  • 0264-9381 (ISSN-L)
  • 1361-6382
OpenAlex
W2062807144
Cited by
116
References
0
Citations by year
2025: 8 · 2024: 9 · 2023: 6 · 2022: 4 · 2021: 6 · 2020: 6 · 2019: 4 · 2018: 6 · 2017: 6 · 2016: 3 · 2015: 2 · 2014: 6 · 2013: 1
FWCI
3.00
Type
journal article
Language
en
Open access
Locations
  • Classical and Quantum Gravity (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
Keywords
quintessential inflation, relic gravitons, gravitational wave background, stochastic gravitational waves, gravitational wave energy spectrum, big bang nucleosynthesis constraints, inflationary models, gravitational wave detection

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