The top documents tagged [gravitational radiation]

t'Hooft General Relativity
Documents t'Hooft General Relativity

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Skript Astrophysics
Documents Skript Astrophysics

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100 Years of General Relativity (2015)
Documents 100 Years of General Relativity (2015)

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The Secondary Stars of Cataclysmic Variables Christian Knigge arXiv:1101.1538v2 reporter:ShaoYong
Documents The Secondary Stars of Cataclysmic Variables Christian Knigge arXiv:1101.1538v2 reporter:ShaoYong

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M. Shara Sept. 26, 2007 Planets, White Dwarfs, Cataclysmic Variables and SNIa in Star Clusters: Changing the Rules Mike Shara American Museum of Natural
Documents M. Shara Sept. 26, 2007 Planets, White Dwarfs, Cataclysmic Variables and SNIa in Star Clusters: Changing the Rules Mike Shara American Museum of Natural

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LIGO Perks Up Its Ears Peter Shawhan Caltech / LIGO Seminars at Maryland, Syracuse, and UMass February / March 2006 LIGO-G060029-00-Z My employer The
Documents LIGO Perks Up Its Ears Peter Shawhan Caltech / LIGO Seminars at Maryland, Syracuse, and UMass February / March 2006 LIGO-G060029-00-Z My employer The

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LIGO-G020224-00-W Gearing Up for Gravitational Waves: Commissioning LIGO Reported on behalf of LIGO colleagues by Fred Raab, LIGO Hanford Observatory
Documents LIGO-G020224-00-W Gearing Up for Gravitational Waves: Commissioning LIGO Reported on behalf of LIGO colleagues by Fred Raab, LIGO Hanford Observatory

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Http://constellation.nasa.gov Beyond Einstein: From the Big Bang to Black Holes Neutron Star Fundamental Physics with Constellation-X ~ 1 x 10 15 g cm
Documents Http://constellation.nasa.gov Beyond Einstein: From the Big Bang to Black Holes Neutron Star Fundamental Physics with Constellation-X ~ 1 x 10 15 g cm

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1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If
Documents 1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If

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1 Einstein's Legacy: General Relativity, our Best Description of the Universe Barry C. Barish Caltech LLNL Science Day 23-May-05
Documents 1 Einstein's Legacy: General Relativity, our Best Description of the Universe Barry C. Barish Caltech LLNL Science Day 23-May-05

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Determining the Equation of State of Ultradense Matter with the Advanced X-ray Timing Array (AXTAR) Deepto Chakrabarty (MIT) Paul S. Ray (NRL) Tod Strohmayer
Documents Determining the Equation of State of Ultradense Matter with the Advanced X-ray Timing Array (AXTAR) Deepto Chakrabarty (MIT) Paul S. Ray (NRL) Tod Strohmayer

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Mike Shara Department of Astrophysics American Museum of Natural History STAR CLUSTER DYNA MIC S Or: BINARY EVOLUTION on STEROIDS
Documents Mike Shara Department of Astrophysics American Museum of Natural History STAR CLUSTER DYNA MIC S Or: BINARY EVOLUTION on STEROIDS

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