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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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Datensatz-Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-DD06-F Versions-Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-DD07-D
Genre: Konferenzbeitrag

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Urheber

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 Urheber:
Gong, Xuefei, Autor
Lau, Yun-Kau, Autor
Xu, Shengnian, Autor
Amaro-Seoane, Pau1, Autor              
Bai, Shan, Autor
Bian, Xing, Autor
Cao, Zhoujian, Autor
Chen, Gerui, Autor
Chen, Xian, Autor
Ding, Yanwei, Autor
Dong, Peng, Autor
Gao, Wei, Autor
Heinzel, Gerhard2, Autor              
Li, Ming, Autor
Li, Shuo, Autor
Liu, Fukun, Autor
Luo, Ziren, Autor
Shao, Mingxue, Autor
Spurzem, Rainer, Autor
Sun, Baosan, Autor
Tang, Wenlin, AutorWang, Yan, AutorXu, Peng, AutorYu, Pin, AutorYuan, Yefei, AutorZhang, Xiaomin, AutorZhou, Zebing, Autor mehr..
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              

Inhalt

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Schlagwörter: 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
 Zusammenfassung: 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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 Datum: 2014-10-222014-11-282015
 Publikationsstatus: Im Druck publiziert
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: -
 Identifikatoren: arXiv: 1410.7296
DOI: 10.1088/1742-6596/610/1/012011
URI: http://arxiv.org/abs/1410.7296
 Art des Abschluß: -

Veranstaltung

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Titel: 10th International LISA Symposium
Veranstaltungsort: Florida, USA
Start-/Enddatum: 2014-05-18 - 2014-05-23

Entscheidung

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Quelle 1

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Titel: Journal of Physics: Conference Series
Genre der Quelle: Zeitschrift
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Affiliations:
Ort, Verlag, Ausgabe: Bristol : IOP Publishing
Seiten: - Band / Heft: 610 Artikelnummer: 012011 Start- / Endseite: - Identifikator: ISSN: 1742-6588
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111097776606042