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Challenges and Opportunities of Gravitational Wave Searches above 10 kHz / Aggarwal, Nancy (Northwestern U.) ; Aguiar, Odylio D. (Sao Jose, INPE) ; Blas, Diego (Barcelona, IFAE ; ICREA, Barcelona) ; Bauswein, Andreas (Darmstadt, GSI) ; Cella, Giancarlo (INFN, Pisa) ; Clesse, Sebastian (Brussels U.) ; Cruise, Adrian Michael (Birmingham U.) ; Domcke, Valerie (CERN) ; Ellis, Sebastian (Geneva U.) ; Figueroa, Daniel G. (Valencia U., IFIC) et al.
The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. [...]
arXiv:2501.11723 ; CERN-TH-2025-014 ; DESY-25-007. - 138.
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Axion Dark Matter / Adams, C.B. (Munich, Max Planck Inst. ; Columbia U.) ; Aggarwal, N. (Northwestern U.) ; Agrawal, A. (Chicago U.) ; Balafendiev, R. (Unlisted) ; Bartram, C. (Washington U., Seattle) ; Baryakhtar, M. (Washington U., Seattle) ; Bekker, H. (Helmholtz Inst., Mainz ; Mainz U.) ; Belov, P. (Unlisted) ; Berggren, K.K. (MIT) ; Berlin, A. (Fermilab) et al.
Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. [...]
arXiv:2203.14923 ; FERMILAB-CONF-22-996-PPD-T. - 96.
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Search for a Dark-Matter-Induced Cosmic Axion Background with ADMX / ADMX Collaboration
We report the first result of a direct search for a Cosmic ${\it axion}$ Background (C$a$B) - a relativistic background of axions that is not dark matter - performed with the axion haloscope, the Axion Dark Matter eXperiment (ADMX). Conventional haloscope analyses search for a signal with a narrow bandwidth, as predicted for dark matter, whereas the C$a$B will be broad. [...]
arXiv:2303.06282; FERMILAB-PUB-23-109-PPD-SQMS; CERN-TH-2023-041.- 2023-09-08 - 7 p. - Published in : Phys. Rev. Lett. 131 (2023) 101002 Fulltext: 2303.06282 - PDF; FERMILAB-PUB-23-109-PPD-SQMS - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server

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New Horizons: Scalar and Vector Ultralight Dark Matter / Antypas, D. (Mainz U. ; Helmholtz Inst., Mainz) ; Banerjee, A. (Weizmann Inst.) ; Bartram, C. (Washington U., Seattle) ; Baryakhtar, M. (Washington U., Seattle) ; Betz, J. (U. Delaware, Newark) ; Bollinger, J.J. (NIST, Boulder) ; Boutan, C. (PNL, Richland) ; Bowring, D. (Fermilab) ; Budker, D. (Helmholtz Inst., Mainz ; Mainz U. ; UC, Berkeley) ; Carney, D. (LBL, Berkeley) et al.
The last decade has seen unprecedented effort in dark matter model building at all mass scales coupled with the design of numerous new detection strategies. [...]
arXiv:2203.14915 ; FERMILAB-PUB-22-262-AD-PPD-T. - 89.
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Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies / Aggarwal, Nancy (Northwestern U.) ; Aguiar, Odylio D. (Sao Jose, INPE) ; Bauswein, Andreas (Darmstadt, GSI) ; Cella, Giancarlo (INFN, Pisa) ; Clesse, Sebastian (Brussels U.) ; Cruise, Adrian Michael (Birmingham U.) ; Domcke, Valerie (Geneva U., Dept. Theor. Phys. ; LPHE, Lausanne ; DESY) ; Figueroa, Daniel G. (Valencia U., IFIC) ; Geraci, Andrew (Northwestern U.) ; Goryachev, Maxim (Western Australia U.) et al.
The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. This white paper outlines the challenges and gains expected in gravitational wave searches at frequencies above the LIGO/Virgo band, with a particular focus on Ultra High-Frequency Gravitational Waves (UHF-GWs), covering the MHz to GHz range. [...]
arXiv:2011.12414; CERN-TH-2020-185; HIP-2020-28/TH; DESY 20-195; CERN-TH-2020-185; HIP-2020-28/TH; DESY 20-195.- 2021-12-06 - 60 p. - Published in : Living Rev. Relativ. 24 (2021) 4 Fulltext: 2011.12414 - PDF; document - PDF;

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Dark Sectors and New, Light, Weakly-Coupled Particles / Essig, Rouven (YITP, Stony Brook) ; Jaros, John A. (SLAC) ; Wester, William (Fermilab) ; Hansson Adrian, P. (SLAC) ; Andreas, S. (DESY ; Paris, Inst. Astrophys.) ; Averett, T. (William-Mary Coll.) ; Baker, O. (Yale U.) ; Batell, B. (Chicago U.) ; Battaglieri, M. (INFN, Genoa) ; Beacham, J. (New York U.) et al.
Dark sectors, consisting of new, light, weakly-coupled particles that do not interact with the known strong, weak, or electromagnetic forces, are a particularly compelling possibility for new physics. [...]
arXiv:1311.0029 ; YITP-SB-36 ; FERMILAB-CONF-13-653. - 2013. - 71 p.
PDF on ECONF - Proceedings write-up on ECONF - Fermilab Library Server (fulltext available) - Full text

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Mechanical Quality Factor Of A Cryogenic Sapphire Test Mass For Gravitational Wave Detectors / Uchiyama, T ; Tomaru, T ; Tobar, M E ; Tatsumi, D ; Miyoki, S ; Ohashi, M ; Kuroda, K ; Suzuki, T ; Sato, N ; Haruyama, T et al.
KEK-99-61. - 1999.
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Measurement of mechanical Q-factors of a cryogenic sapphire test mass for laser interferometric gravitational wave detectors / Uchiyama, T ; Tomaru, T ; Tobar, M E ; Tatsumi, D ; Miyoki, S ; Kuroda, K ; Suzuki, T ; Sato, N ; Haruyama, T ; Yamamoto, A et al.
ICRR-444. - 1999. - 12 p.
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Search for gravitational waves from the millisecond pulsar PSR 0437-471 / Mohanty, S D ; Heng, I S ; Blair, D G ; Dhurandhar, S V ; Tobar, M E ; Ivanov, E
IUCAA-98-14. - 1998. - 30 p.
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10.

Cryogenic cooling of a sapphire mirror-suspension for interferometric gravitational wave detectors / Uchiyama, T ; Tatsumi, D ; Tomaru, T ; Tobar, M E ; Kuroda, K ; Suzuki, T ; Sato, N ; Yamamoto, A ; Haruyama, T ; Shintomi, T
ICRR-410. - 1998. - 9 p.
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Vea también: autores con nombres similares
3	Tobar, M
41	Tobar, M E
26	Tobar, M J
2	Tobar, M.
4	Tobar, M.J.
8	Tobar, Michael
37	Tobar, Michael E
2	Tobar, Michael E.
11	Tobar, Michael Edmund

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