(Q63391148)

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Signal-to-noise ratio for a stochastic background of massive relic particles

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title

Signal-to-noise ratio for a stochastic background of massive relic particles (English)

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M. Gasperini

1

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publication date

March 2000

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published in

Physics Letters B

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volume

477

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issue

1-3

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page(s)

242-247

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cites work

Sensitivity of the Laser Interferometer Gravitational Wave Observatory to a stochastic background, and its dependence on the detector orientations

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https://api.crossref.org/works/10.1016%2FS0370-2693%2800%2900195-7

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7 January 2021

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Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities

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https://api.crossref.org/works/10.1016%2FS0370-2693%2800%2900195-7

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7 January 2021

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On the response of gravitational antennas to dilatonic waves

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https://api.crossref.org/works/10.1016%2FS0370-2693%2800%2900195-7

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7 January 2021

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Six years of the fifth force

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https://api.crossref.org/works/10.1016%2FS0370-2693%2800%2900195-7

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7 January 2021

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Constraints on pre-big-bang models for seeding large-scale anisotropy by massive Kalb-Ramond axions

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https://api.crossref.org/works/10.1016%2FS0370-2693%2800%2900195-7

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7 January 2021

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Metric perturbations in dilaton-driven inflation

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https://api.crossref.org/works/10.1016%2FS0370-2693%2800%2900195-7

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7 January 2021

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Identifiers

DOI

10.1016/S0370-2693(00)00195-7

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arXiv ID

gr-qc/0001094

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(Q63391148)

Signal-to-noise ratio for a stochastic background of massive relic particles

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