A scientific case study of an advanced LISA mission
暂无分享,去创建一个
Xuefei Gong | Yan Wang | Peng Xu | Rainer Spurzem | Ziren Luo | Gerhard Heinzel | Hsien-Chi Yeh | Yanbei Chen | Ze-Bing Zhou | Mingxue Shao | Yun-Kau Lau | Shengnian Xu | Gerui Chen | G. Heinzel | S. Bai | H. Yeh | Yanbei Chen | R. Spurzem | P. Xu | Zhoujian Cao | X. Gong | Ziren Luo | Shengnian Xu | Y. Lau | A. P. Patón | Xiao He | Antonio Pulido Paton | Zhoujian Cao | Jun Luo | Albrecht Ruediger | Shan Bai | Xiao-Kai He | Chenzhou Liu | Y. Yuan | Chenzhou Liu | Zebing Zhou | Yan Wang | A. Ruediger | Jun Luo | Mingxue Shao | Gerui Chen | Y. Yuan
[1] J. Gair,et al. Exploring intermediate and massive black-hole binaries with the Einstein Telescope , 2009, 0907.5450.
[2] S. E. Woosley,et al. The Nucleosynthetic Signature of Population III , 2002 .
[3] N. Cornish,et al. Beyond LISA: Exploring future gravitational wave missions , 2005, gr-qc/0506015.
[4] P. Ajith,et al. Template bank for gravitational waveforms from coalescing binary black holes: Nonspinning binaries , 2008 .
[5] R. DeSalvo,et al. A xylophone configuration for a third-generation gravitational wave detector , 2009, 0906.2655.
[6] The Distribution and cosmic evolution of massive black hole spins , 2004, astro-ph/0410342.
[7] A. Heptonstall,et al. Increased Brownian force noise from molecular impacts in a constrained volume. , 2009, Physical review letters.
[8] Alberto Sesana,et al. The imprint of massive black hole formation models on the LISA data stream , 2007, astro-ph/0701556.
[9] E. Colbert,et al. Observational Evidence for Intermediate-Mass Black Holes in Ultra-luminous X-ray Sources , 2004, astro-ph/0402677.
[10] Gravitational Radiation from Intermediate-Mass Black Holes , 2002, astro-ph/0206404.
[11] Piero Madau,et al. The formation of galaxy stellar cores by the hierarchical merging of supermassive black holes , 2003 .
[12] F. Ohme,et al. "Complete" gravitational waveforms for black-hole binaries with non-precessing spins , 2010 .
[13] Clifford M. Will,et al. On the Rate of Detectability of Intermediate-Mass Black Hole Binaries Using LISA , 2004, astro-ph/0403644.
[14] A. University,et al. Massive black hole seeds from low angular momentum material , 2003, astro-ph/0311487.
[15] Piero Madau,et al. The Assembly and Merging History of Supermassive Black Holes in Hierarchical Models of Galaxy Formation , 2002, astro-ph/0207276.
[16] Simon F. Portegies Zwart,et al. The Runaway Growth of Intermediate-Mass Black Holes in Dense Star Clusters , 2002, astro-ph/0201055.
[17] A. Sesana. Extreme recoils: impact on the detection of gravitational waves from massive black hole binaries , 2007, 0707.4677.
[18] T Nakamura,et al. Possibility of direct measurement of the acceleration of the universe using 0.1 Hz band laser interferometer gravitational wave antenna in space. , 2001, Physical review letters.
[19] S. Larson,et al. Sensitivity curves for spaceborne gravitational wave interferometers , 1999, gr-qc/9909080.
[20] W. Del Pozzo,et al. Triple Michelson interferometer for a third-generation gravitational wave detector , 2008, 0804.1036.