Zobrazeno 1 - 10
of 326
pro vyhledávání: '"Boggs, William"'
Publikováno v:
Physical Review D 84:084009 (2011)
We conduct a descriptive analysis of the multipolar structure of gravitational-radiation waveforms from equal-mass aligned-spin mergers, following an approach first presented in the complementary context of nonspinning black holes of varying mass rat
Externí odkaz:
http://arxiv.org/abs/1107.1181
Autor:
van Meter, James R., Miller, M. Coleman, Baker, John G., Boggs, William D., Kelly, Bernard J.
Although the gravitational wave kick velocity in the orbital plane of coalescing black holes has been understood for some time, apparently conflicting formulae have been proposed for the dominant out-of-plane kick, each a good fit to different data s
Externí odkaz:
http://arxiv.org/abs/1003.3865
Autor:
van Meter, James R., Wise, John H., Miller, M. Coleman, Reynolds, Christopher S., Centrella, Joan M., Baker, John G., Boggs, William D., Kelly, Bernard J., McWilliams, Sean T.
Publikováno v:
Astrophys.J.711:L89,2010
Coalescing massive black hole binaries are produced by the mergers of galaxies. The final stages of the black hole coalescence produce strong gravitational radiation that can be detected by the space-borne LISA. In cases where the black hole merger t
Externí odkaz:
http://arxiv.org/abs/0908.0023
Autor:
Aylott, Benjamin, Baker, John G., Boggs, William D., Boyle, Michael, Brady, Patrick R., Brown, Duncan A., Brügmann, Bernd, Buchman, Luisa T., Buonanno, Alessandra, Cadonati, Laura, Camp, Jordan, Campanelli, Manuela, Centrella, Joan, Chatterjis, Shourov, Christensen, Nelson, Chu, Tony, Diener, Peter, Dorband, Nils, Etienne, Zachariah B., Faber, Joshua, Fairhurst, Stephen, Farr, Benjamin, Fischetti, Sebastian, Guidi, Gianluca, Goggin, Lisa M., Hannam, Mark, Herrmann, Frank, Hinder, Ian, Husa, Sascha, Kalogera, Vicky, Keppel, Drew, Kidder, Lawrence E., Kelly, Bernard J., Krishnan, Badri, Laguna, Pablo, Lousto, Carlos O., Mandel, Ilya, Marronetti, Pedro, Matzner, Richard, McWilliams, Sean T., Matthews, Keith D., Mercer, R. Adam, Mohapatra, Satyanarayan R. P., Mroué, Abdul H., Nakano, Hiroyuki, Ochsner, Evan, Pan, Yi, Pekowsky, Larne, Pfeiffer, Harald P., Pollney, Denis, Pretorius, Frans, Raymond, Vivien, Reisswig, Christian, Rezzolla, Luciano, Rinne, Oliver, Robinson, Craig, Röver, Christian, Santamaría, Lucía, Sathyaprakash, Bangalore, Scheel, Mark A., Schnetter, Erik, Seiler, Jennifer, Shapiro, Stuart L., Shoemaker, Deirdre, Sperhake, Ulrich, Stroeer, Alexander, Sturani, Riccardo, Tichy, Wolfgang, Liu, Yuk Tung, van der Sluys, Marc, van Meter, James R., Vaulin, Ruslan, Vecchio, Alberto, Veitch, John, Viceré, Andrea, Whelan, John T., Zlochower, Yosef
Publikováno v:
Class.Quant.Grav.26:114008,2009
The 2008 NRDA conference introduced the Numerical INJection Analysis project (NINJA), a new collaborative effort between the numerical relativity community and the data analysis community. NINJA focuses on modeling and searching for gravitational wav
Externí odkaz:
http://arxiv.org/abs/0905.4227
Autor:
Aylott, Benjamin, Baker, John G., Boggs, William D., Boyle, Michael, Brady, Patrick R., Brown, Duncan A., Brügmann, Bernd, Buchman, Luisa T., Buonanno, Alessandra, Cadonati, Laura, Camp, Jordan, Campanelli, Manuela, Centrella, Joan, Chatterji, Shourov, Christensen, Nelson, Chu, Tony, Diener, Peter, Dorband, Nils, Etienne, Zachariah B., Faber, Joshua, Fairhurst, Stephen, Farr, Benjamin, Fischetti, Sebastian, Guidi, Gianluca, Goggin, Lisa M., Hannam, Mark, Herrmann, Frank, Hinder, Ian, Husa, Sascha, Kalogera, Vicky, Keppel, Drew, Kidder, Lawrence E., Kelly, Bernard J., Krishnan, Badri, Laguna, Pablo, Lousto, Carlos O., Mandel, Ilya, Marronetti, Pedro, Matzner, Richard, McWilliams, Sean T., Matthews, Keith D., Mercer, R. Adam, Mohapatra, Satyanarayan R. P., Mroué, Abdul H., Nakano, Hiroyuki, Ochsner, Evan, Pan, Yi, Pekowsky, Larne, Pfeiffer, Harald P., Pollney, Denis, Pretorius, Frans, Raymond, Vivien, Reisswig, Christian, Rezzolla, Luciano, Rinne, Oliver, Robinson, Craig, Röver, Christian, Santamaría, Lucía, Sathyaprakash, Bangalore, Scheel, Mark A., Schnetter, Erik, Seiler, Jennifer, Shapiro, Stuart L., Shoemaker, Deirdre, Sperhake, Ulrich, Stroeer, Alexander, Sturani, Riccardo, Tichy, Wolfgang, Liu, Yuk Tung, van der Sluys, Marc, van Meter, James R., Vaulin, Ruslan, Vecchio, Alberto, Veitch, John, Viceré, Andrea, Whelan, John T., Zlochower, Yosef
Publikováno v:
Class.Quant.Grav.26:165008,2009
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/0901.4399
Kniha
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Baker, John G., Boggs, William D., Centrella, Joan, Kelly, Bernard J., McWilliams, Sean T., van Meter, James R.
Publikováno v:
Phys.Rev.D78:044046,2008
We present a detailed descriptive analysis of the gravitational radiation from black-hole binary mergers of nonspinning black holes, based on numerical simulations of systems varying from equal-mass to a 6:1 mass ratio. Our primary goal is to present
Externí odkaz:
http://arxiv.org/abs/0805.1428
Autor:
Baker, John G., Boggs, William D., Centrella, Joan, Kelly, Bernard J., McWilliams, Sean T., Miller, M. Coleman, van Meter, James R.
Publikováno v:
Astrophys.J.682:L29-L32,2008
Recent numerical relativistic results demonstrate that the merger of comparable-mass spinning black holes has a maximum ``recoil kick'' of up to $\sim 4000 \kms$. However the scaling of these recoil velocities with mass ratio is poorly understood. We
Externí odkaz:
http://arxiv.org/abs/0802.0416
Autor:
Baker, John G., Boggs, William D., Centrella, Joan M., Kelly, Bernard J., McWilliams, Sean T., van Meter, James R.
Coalescing black-hole binaries are expected to be the strongest sources of gravitational waves for ground-based interferometers as well as the space-based interferometer LISA. Recent progress in numerical relativity now makes it possible to calculate
Externí odkaz:
http://arxiv.org/abs/0708.4202