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01220nam a2200145Ia 4500 |
| 001 |
10.1103-PhysRevD.105.083001 |
| 008 |
220510s2022 CNT 000 0 und d |
| 020 |
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|a 24700010 (ISSN)
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| 245 |
1 |
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|a Detection prospects of dark matter in the Einstein Telescope
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| 260 |
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|b American Physical Society
|c 2022
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| 856 |
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|z View Fulltext in Publisher
|u https://doi.org/10.1103/PhysRevD.105.083001
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| 520 |
3 |
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|a We improve the calculations of the elastic motion induced by dark matter hitting the surface of the mirror inside an interferometer used for gravitational-wave detection. We focus on the discovery potential of such a dark matter signal in the third-generation European gravitational-wave detector, the Einstein Telescope. By taking the thickness of the mirror into account, more than one resonance is predicted in the sensitive regime of the high-frequency interferometer. When the mass of dark matter is heavier than a few PeV or is highly boosted, the signal-to-noise ratio could exceed one, and the Einstein Telescope should be able to detect this dark matter signal. © 2022 authors. Published by the American Physical Society.
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| 700 |
1 |
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|a Chen, C.-R.
|e author
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| 700 |
1 |
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|a Nugroho, C.S.
|e author
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| 773 |
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|t Physical Review D
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