Details
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | L061303 |
| Fachzeitschrift | Physical Review D |
| Jahrgang | 108 |
| Ausgabenummer | 6 |
| Publikationsstatus | Veröffentlicht - 20 Sept. 2023 |
Abstract
High frequency gravitational waves can be detected by observing the frequency modulation they impart on photons. We discuss fundamental limitations to this method related to the fact that it is impossible to construct a perfectly rigid detector. We then propose several novel methods to search for O(MHz-GHz) gravitational waves based on the frequency modulation induced in the spectrum of an intense laser beam, by applying optical frequency demodulation techniques, or by using optical atomic clock technology. We find promising sensitivities across a broad frequency range.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Kern- und Hochenergiephysik
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in: Physical Review D, Jahrgang 108, Nr. 6, L061303, 20.09.2023.
Publikation: Beitrag in Fachzeitschrift › Letter › Forschung › Peer-Review
}
TY - JOUR
T1 - High-frequency gravitational wave detection via optical frequency modulation
AU - Bringmann, Torsten
AU - Domcke, Valerie
AU - Fuchs, Elina
AU - Kopp, Joachim
N1 - Funding Information: It is a pleasure to thank Wolfram Ratzinger for very illuminating discussions on the Doppler shift of photons in a GW background, Johannes Skaar for educating us on Bragg filters and fiber optics in general, Jun Ye for innumerable crucial insights into the physics of atomic clocks, Fritz Wagner for sharing his expertise on the Mössbauer effect, Klemens Hammerer for useful explanations on sideband detection with cavities, Tom Melia, Piet Schmidt, and Tadahiro Takahashi for illuminating discussions on optical clock comparisons, Lingze Duan for important insights on optical demodulation, Camilo Garcia Cely, Sebastian Ellis, Sung Mook Lee, and Nick Rodd for their insights on comparing high frequency GW sensitivities as well as on the quirks of the proper detector frame, and Clara Murgui for her explanations around optomechanical cavities. We moreover thank Camilo Garcia Cely, Lingze Duan, Klemens Hammerer, and Tadahiro Takahashi for valuable comments on the manuscript. E. F. acknowledges support by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy—EXC-2123 “QuantumFrontiers”—390837967.
PY - 2023/9/20
Y1 - 2023/9/20
N2 - High frequency gravitational waves can be detected by observing the frequency modulation they impart on photons. We discuss fundamental limitations to this method related to the fact that it is impossible to construct a perfectly rigid detector. We then propose several novel methods to search for O(MHz-GHz) gravitational waves based on the frequency modulation induced in the spectrum of an intense laser beam, by applying optical frequency demodulation techniques, or by using optical atomic clock technology. We find promising sensitivities across a broad frequency range.
AB - High frequency gravitational waves can be detected by observing the frequency modulation they impart on photons. We discuss fundamental limitations to this method related to the fact that it is impossible to construct a perfectly rigid detector. We then propose several novel methods to search for O(MHz-GHz) gravitational waves based on the frequency modulation induced in the spectrum of an intense laser beam, by applying optical frequency demodulation techniques, or by using optical atomic clock technology. We find promising sensitivities across a broad frequency range.
UR - http://www.scopus.com/inward/record.url?scp=85172917496&partnerID=8YFLogxK
U2 - 10.48550/arXiv.2304.10579
DO - 10.48550/arXiv.2304.10579
M3 - Letter
AN - SCOPUS:85172917496
VL - 108
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 6
M1 - L061303
ER -