Standard

Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton to photon conversion. / Ejlli, A.; Ejlli, D.; Cruise, A. M. et al.

In: European Physical Journal C, Vol. 79, No. 12, 1032, 01.12.2019.

Research output: Contribution to journalArticlepeer-review

Harvard

Ejlli, A, Ejlli, D, Cruise, AM, Pisano, G & Grote, H 2019, 'Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton to photon conversion', European Physical Journal C, vol. 79, no. 12, 1032. https://doi.org/10.1140/epjc/s10052-019-7542-5

APA

Ejlli, A., Ejlli, D., Cruise, A. M., Pisano, G., & Grote, H. (2019). Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton to photon conversion. European Physical Journal C, 79(12), [1032]. https://doi.org/10.1140/epjc/s10052-019-7542-5

Vancouver

Ejlli A, Ejlli D, Cruise AM, Pisano G, Grote H. Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton to photon conversion. European Physical Journal C. 2019 Dec 1;79(12):1032. doi: 10.1140/epjc/s10052-019-7542-5

Author

Ejlli, A. ; Ejlli, D. ; Cruise, A. M. et al. / Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton to photon conversion. In: European Physical Journal C. 2019 ; Vol. 79, No. 12.

BibTeX

@article{47f51031aec745d2aab170413910132e,
title = "Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton to photon conversion",
abstract = "In this work, we present the first experimental upper limits on the presence of stochastic gravitational waves in a frequency band with frequencies above 1 THz. We exclude gravitational waves in the frequency bands from (2.7 - 14) × 10 14 Hz and (5 - 12) × 10 18 Hz down to a characteristic amplitude of hcmin≈6×10-26 and hcmin≈5×10-28 at 95% confidence level, respectively. To obtain these results, we used data from existing facilities that have been constructed and operated with the aim of detecting weakly interacting slim particles, pointing out that these facilities are also sensitive to gravitational waves by graviton to photon conversion in the presence of a magnetic field. The principle applies to all experiments of this kind, with prospects of constraining (or detecting), for example, gravitational waves from light primordial black-hole evaporation in the early universe.",
keywords = "BLACK-HOLE",
author = "A. Ejlli and D. Ejlli and Cruise, {A. M.} and G. Pisano and H. Grote",
year = "2019",
month = dec,
day = "1",
doi = "10.1140/epjc/s10052-019-7542-5",
language = "English",
volume = "79",
journal = "European Physical Journal C",
issn = "1434-6044",
publisher = "Springer Nature",
number = "12",

}

RIS

TY - JOUR

T1 - Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton to photon conversion

AU - Ejlli, A.

AU - Ejlli, D.

AU - Cruise, A. M.

AU - Pisano, G.

AU - Grote, H.

PY - 2019/12/1

Y1 - 2019/12/1

N2 - In this work, we present the first experimental upper limits on the presence of stochastic gravitational waves in a frequency band with frequencies above 1 THz. We exclude gravitational waves in the frequency bands from (2.7 - 14) × 10 14 Hz and (5 - 12) × 10 18 Hz down to a characteristic amplitude of hcmin≈6×10-26 and hcmin≈5×10-28 at 95% confidence level, respectively. To obtain these results, we used data from existing facilities that have been constructed and operated with the aim of detecting weakly interacting slim particles, pointing out that these facilities are also sensitive to gravitational waves by graviton to photon conversion in the presence of a magnetic field. The principle applies to all experiments of this kind, with prospects of constraining (or detecting), for example, gravitational waves from light primordial black-hole evaporation in the early universe.

AB - In this work, we present the first experimental upper limits on the presence of stochastic gravitational waves in a frequency band with frequencies above 1 THz. We exclude gravitational waves in the frequency bands from (2.7 - 14) × 10 14 Hz and (5 - 12) × 10 18 Hz down to a characteristic amplitude of hcmin≈6×10-26 and hcmin≈5×10-28 at 95% confidence level, respectively. To obtain these results, we used data from existing facilities that have been constructed and operated with the aim of detecting weakly interacting slim particles, pointing out that these facilities are also sensitive to gravitational waves by graviton to photon conversion in the presence of a magnetic field. The principle applies to all experiments of this kind, with prospects of constraining (or detecting), for example, gravitational waves from light primordial black-hole evaporation in the early universe.

KW - BLACK-HOLE

UR - http://www.scopus.com/inward/record.url?scp=85077025312&partnerID=8YFLogxK

U2 - 10.1140/epjc/s10052-019-7542-5

DO - 10.1140/epjc/s10052-019-7542-5

M3 - Article

AN - SCOPUS:85077025312

VL - 79

JO - European Physical Journal C

JF - European Physical Journal C

SN - 1434-6044

IS - 12

M1 - 1032

ER -

ID: 23090048