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Laser Interferometer Space Antenna
/ LISA Collaboration
Following the selection of The Gravitational Universe by ESA, and the successful flight of LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's call for missions for L3. [...]
arXiv:1702.00786.
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2017. - 41 p.
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LISA Definition Study Report
/ Colpi, Monica (INFN, Milan Bicocca) ; Danzmann, Karsten (Hannover, Max Planck Inst. Grav.) ; Hewitson, Martin (Hannover, Max Planck Inst. Grav.) ; Jetzer, Philippe (U. Zurich (main)) ; Nelemans, Gijs (Nijmegen U., IMAPP) ; Petiteau, Antoine (IRFU, Saclay) ; Shoemaker, David (MIT, MKI) ; Sopuerta, Carlos (ICE, Bellaterra) ; Stebbins, Robin (Colorado U.) ; Tanvir, Nial (Leicester U.) et al.
The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. [...]
arXiv:2402.07571.
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155.
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STE-QUEST: Space Time Explorer and QUantum Equivalence principle Space Test
/ STE-QUEST Collaboration
An M-class mission proposal in response to the 2021 call in ESA's science programme with a broad range of objectives in fundamental physics, which include testing the Equivalence Principle and Lorentz Invariance, searching for Ultralight Dark Matter and probing Quantum Mechanics..
arXiv:2211.15412 ; CERN-TH-2022-202.
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78 p.
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Gravitational Wave Data Analysis: Computing Challenges in the 3G Era
/ Couvares, Peter (Caltech, Pasadena (main)) ; Bird, Ian (CERN) ; Porter, Edward (APC, Paris) ; Bagnasco, Stefano (INFN, Italy) ; Lovelace, Geoffrey (Cal State, Fullerton) ; Punturo, Michele (INFN, Perugia) ; Reitze, David (Caltech, Pasadena (main)) ; Katsanevas, Stavros (EGO, Pisa) ; Kajita, Takaaki (Tokyo U.) ; Kalogera, Vicky (Northwestern U.) et al.
Cyber infrastructure will be a critical consideration in the development of next generation gravitational-wave detectors. [...]
arXiv:2111.06987.
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26 p.
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Tests of General Relativity with GWTC-3
/ LIGO Scientific Collaboration
The ever-increasing number of detections of gravitational waves (GWs) from compact binaries by the Advanced LIGO and Advanced Virgo detectors allows us to perform ever-more sensitive tests of general relativity (GR) in the dynamical and strong-field regime of gravity. [...]
arXiv:2112.06861 ; LIGO-P2100275.
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41 p.
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Bayesian versus frequentist upper limits
/ Rover, Christian (Hannover, Max Planck Inst. Grav.) ; Messenger, Chris (Hannover, Max Planck Inst. Grav. ; Cardiff U.) ; Prix, Reinhard (Hannover, Max Planck Inst. Grav.)
While gravitational waves have not yet been measured directly, data analysis from detection experiments commonly includes an upper limit statement. Such upper limits may be derived via a frequentist or Bayesian approach; the theoretical implications are very different, and on the technical side, one notable difference is that one case requires maximization of the likelihood function over parameter space, while the other requires integration. [...]
arXiv:1103.2987; AEI-2011-014; AEI-2011-014.-
Geneva : CERN, 2011 - 6 p.
- Published in : 10.5170/CERN-2011-006.158
Fulltext: 1087459_158-163 - PDF; arXiv:1103.2987 - PDF; External link: Preprint
In : Proceedings of the PHYSTAT 2011 Workshop on Statistical Issues Related to Discovery Claims in Search Experiments and Unfolding, pp.158-163
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EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade
/ Alves Batista, R. (Madrid, IFT) ; Amin, M.A. (Rice U.) ; Barenboim, G. (Valencia U.) ; Bartolo, N. (U. Padua, Dept. Phys. Astron.) ; Baumann, D. (Amsterdam U. ; U. Amsterdam, GRAPPA ; U. Edinburgh, Higgs Ctr. Theor. Phys.) ; Bauswein, A. (Darmstadt, GSI) ; Bellini, E. (Geneva U., Dept. Theor. Phys.) ; Benisty, D. (Cambridge U., DAMTP ; Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; Bertone, G. (Amsterdam U. ; U. Amsterdam, GRAPPA) ; Blasi, P. (GSSI, Aquila ; Gran Sasso) et al.
Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the direct detection of gravitational waves with LIGO and Virgo, and many others. [...]
arXiv:2110.10074.
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134.
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Event rate estimates for LISA extreme mass ratio capture sources
/ Gair, J R (Caltech) ; Barack, L (Texas U., Brownsville, CGWA) ; Creighton, T (LIGO Lab., Caltech) ; Cutler, C (Hannover, Max Planck Inst. Grav.) ; Larson, S L (Caltech, SRL) ; Phinney, E S (Caltech) ; Vallisneri, M (Caltech, JPL)
One of the most exciting prospects for the LISA gravitational wave observatory is the detection of gravitational radiation from the inspiral of a compact object into a supermassive black hole. The large inspiral parameter space and low amplitude of the signal makes detection of these sources computationally challenging. [...]
gr-qc/0405137.-
2004 - 11 p.
- Published in : Class. Quantum Gravity 21 (2004) S1595-S1606
Access to fulltext document: PDF; External link: gr-qc/0405137 PDF
In : 8th Gravitational Wave Data Analysis Workshop, Milwaukee, MI, USA, 17 - 20 Dec 2003, pp.S1595-S1606
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