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pro vyhledávání: '"Müller, Doreen"'
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Autor:
Hinder, Ian, Buonanno, Alessandra, Boyle, Michael, Etienne, Zachariah B., Healy, James, Johnson-McDaniel, Nathan K., Nagar, Alessandro, Nakano, Hiroyuki, Pan, Yi, Pfeiffer, Harald P., Pürrer, Michael, Reisswig, Christian, Scheel, Mark A., Schnetter, Erik, Sperhake, Ulrich, Szilágyi, Bela, Tichy, Wolfgang, Wardell, Barry, Zenginoglu, Anıl, Alic, Daniela, Bernuzzi, Sebastiano, Bode, Tanja, Brügmann, Bernd, Buchman, Luisa T., Campanelli, Manuela, Chu, Tony, Damour, Thibault, Grigsby, Jason D., Hannam, Mark, Haas, Roland, Hemberger, Daniel A., Husa, Sascha, Kidder, Lawrence E., Laguna, Pablo, London, Lionel, Lovelace, Geoffrey, Lousto, Carlos O., Marronetti, Pedro, Matzner, Richard A., Mösta, Philipp, Mroué, Abdul, Müller, Doreen, Mundim, Bruno C., Nerozzi, Andrea, Paschalidis, Vasileios, Pollney, Denis, Reifenberger, George, Rezzolla, Luciano, Shapiro, Stuart L., Shoemaker, Deirdre, Taracchini, Andrea, Taylor, Nicholas W., Teukolsky, Saul A., Thierfelder, Marcus, Witek, Helvi, Zlochower, Yosef
Publikováno v:
Class. Quantum Grav. 31 (2014) 025012
The Numerical-Relativity-Analytical-Relativity (NRAR) collaboration is a joint effort between members of the numerical relativity, analytical relativity and gravitational-wave data analysis communities. The goal of the NRAR collaboration is to produc
Externí odkaz:
http://arxiv.org/abs/1307.5307
Autor:
Ajith, P., Boyle, Michael, Brown, Duncan A., Brügmann, Bernd, Buchman, Luisa T., Cadonati, Laura, Campanelli, Manuela, Chu, Tony, Etienne, Zachariah B., Fairhurst, Stephen, Hannam, Mark, Healy, James, Hinder, Ian, Husa, Sascha, Kidder, Lawrence E., Krishnan, Badri, Laguna, Pablo, Liu, Yuk Tung, London, Lionel, Lousto, Carlos O., Lovelace, Geoffrey, MacDonald, Ilana, Marronetti, Pedro, Mohapatra, Satya, Mösta, Philipp, Müller, Doreen, Mundim, Bruno C., Nakano, Hiroyuki, Ohme, Frank, Paschalidis, Vasileios, Pekowsky, Larne, Pollney, Denis, Pfeiffer, Harald P., Ponce, Marcelo, Pürrer, Michael, Reifenberger, George, Reisswig, Christian, Santamaría, Lucía, Scheel, Mark A., Shapiro, Stuart L., Shoemaker, Deirdre, Sopuerta, Carlos F., Sperhake, Ulrich, Szilágyi, Béla, Taylor, Nicholas W., Tichy, Wolfgang, Tsatsin, Petr, Zlochower, Yosef
The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational wave data analysis communities. The purpose of NINJA is to study the sensitivity of existing gravitational-wave s
Externí odkaz:
http://arxiv.org/abs/1201.5319
We analyse an eleven-orbit inspiral of a non-spinning black-hole binary with mass ratio q=M1/M2=4. The numerically obtained gravitational waveforms are compared with post-Newtonian (PN) predictions including several sub-dominant multipoles up to mult
Externí odkaz:
http://arxiv.org/abs/1012.3173
Publikováno v:
Phys.Rev.D82:124008,2010
We present gravitational waveforms for the last orbits and merger of black-hole-binary (BBH) systems along two branches of the BBH parameter space: equal-mass binaries with equal non-precessing spins, and nonspinning unequal-mass binaries. The wavefo
Externí odkaz:
http://arxiv.org/abs/1007.4789
Publikováno v:
Phys. Rev. D 82, 064004 (2010)
Certain numerical frameworks used for the evolution of binary black holes make use of a gamma driver, which includes a damping factor. Such simulations typically use a constant value for damping. However, it has been found that very specific values o
Externí odkaz:
http://arxiv.org/abs/1003.4681
Autor:
Mueller, Doreen, Bruegmann, Bernd
Publikováno v:
Class.Quant.Grav.27:114008,2010
Moving puncture simulations of black hole binaries rely on a specific gauge choice that leads to approximately stationary coordinates near each black hole. Part of the shift condition is a damping parameter, which has to be properly chosen for stable
Externí odkaz:
http://arxiv.org/abs/0912.3125
Publikováno v:
Phys.Rev.D79:124040,2009
Black hole binaries on non-eccentric orbits form an important subclass of gravitational wave sources, but it is a non-trivial issue to construct numerical initial data with minimal initial eccentricity for numerical simulations. We compute post-Newto
Externí odkaz:
http://arxiv.org/abs/0901.0993