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  Descope of the ALIA mission

Gong, X., Lau, Y.-K., Xu, S., Amaro-Seoane, P., Bai, S., Bian, X., et al. (2015). Descope of the ALIA mission. Journal of Physics: Conference Series, 610: 012011.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-DD06-F Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-DD07-D
Genre: Conference Paper

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 Creators:
Gong, Xuefei, Author
Lau, Yun-Kau, Author
Xu, Shengnian, Author
Amaro-Seoane, Pau1, Author              
Bai, Shan, Author
Bian, Xing, Author
Cao, Zhoujian, Author
Chen, Gerui, Author
Chen, Xian, Author
Ding, Yanwei, Author
Dong, Peng, Author
Gao, Wei, Author
Heinzel, Gerhard2, Author              
Li, Ming, Author
Li, Shuo, Author
Liu, Fukun, Author
Luo, Ziren, Author
Shao, Mingxue, Author
Spurzem, Rainer, Author
Sun, Baosan, Author
Tang, Wenlin, AuthorWang, Yan, AuthorXu, Peng, AuthorYu, Pin, AuthorYuan, Yefei, AuthorZhang, Xiaomin, AuthorZhou, Zebing, Author more..
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              
2Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24010              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE, Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM
 Abstract: The present work reports on a feasibility study commissioned by the Chinese Academy of Sciences of China to explore various possible mission options to detect gravitational waves in space alternative to that of the eLISA/LISA mission concept. Based on the relative merits assigned to science and technological viability, a few representative mission options descoped from the ALIA mission are considered. A semi-analytic Monte Carlo simulation is carried out to understand the cosmic black hole merger histories starting from intermediate mass black holes at high redshift as well as the possible scientific merits of the mission options considered in probing the light seed black holes and their coevolution with galaxies in early Universe. The study indicates that, by choosing the armlength of the interferometer to be three million kilometers and shifting the sensitivity floor to around one-hundredth Hz, together with a very moderate improvement on the position noise budget, there are certain mission options capable of exploring light seed, intermediate mass black hole binaries at high redshift that are not readily accessible to eLISA/LISA, and yet the technological requirements seem to within reach in the next few decades for China.

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 Dates: 2014-10-222014-11-282015
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1410.7296
DOI: 10.1088/1742-6596/610/1/012011
URI: http://arxiv.org/abs/1410.7296
 Degree: -

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Title: 10th International LISA Symposium
Place of Event: Florida, USA
Start-/End Date: 2014-05-18 - 2014-05-23

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Title: Journal of Physics: Conference Series
Source Genre: Journal
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Publ. Info: Bristol : IOP Publishing
Pages: - Volume / Issue: 610 Sequence Number: 012011 Start / End Page: - Identifier: ISSN: 1742-6588
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111097776606042