The effect of mission duration on LISA science objectives
文献类型：期刊论文
| 作者 | Seoane, Pau Amaro1,2,3,4; Sedda, Manuel Arca5; Babak, Stanislav6,7; Berry, Christopher P. L.8,9; Berti, Emanuele10; Bertone, Gianfranco11,12; Blas, Diego13,14,15; Bogdanovic, Tamara16,17; Bonetti, Matteo18; Breivik, Katelyn19 |
| 刊名 | GENERAL RELATIVITY AND GRAVITATION
 |
| 出版日期 | 2022 |
| 卷号 | 54期号:1页码:47 |
| 关键词 | General relativity Gravitational waves Black holes |
| ISSN号 | 0001-7701 |
| DOI | 10.1007/s10714-021-02889-x |
| 英文摘要 | The science objectives of the LISA mission have been defined under the implicit assumption of a 4-years continuous data stream. Based on the performance of LISA Pathfinder, it is now expected that LISA will have a duty cycle of approximate to 0.75, which would reduce the effective span of usable data to 3 years. This paper reports the results of a study by the LISA Science Group, which was charged with assessing the additional science return of increasing the mission lifetime. We explore various observational scenarios to assess the impact of mission duration on the main science objectives of the mission. We find that the science investigations most affected by mission duration concern the search for seed black holes at cosmic dawn, as well as the study of stellar-origin black holes and of their formation channels via multi-band and multi-messenger observations. We conclude that an extension to 6 years of mission operations is recommended. |
| 资助项目 | CIERA Board of Visitors Professorship ; NSF[PHY1912550] ; NSF[AST-2006538] ; NSF[PHY-20043] ; NSF[1908042] ; NSF[AST-2006176] ; NSF[AST-1715661] ; NSF[PHY-1806776] ; NSF[PHY-1912578] ; NASA ATP[17-ATP17-0225] ; NASA ATP[19-ATP19-0051] ; NSF-XSEDE[PHY-090003] ; Fundacion Jesus Serra ; Instituto de Astrofisica de Canarias under the Visiting Researcher Programme 2021 ; National Aeronautics and Space Administration (NASA)[80NSSC19K0319] ; European Union's H2020 ERC Consolidator Grant Matter and strong-field gravity: New frontiers in Einstein's theory[MaGRaTh-646597] ; European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant[101007855] ; FCT[UIDB/00099/2020] ; FCT[PTDC/MAT-APL/30043/2017] ; FCT[PTDC/FIS-AST/7002/2020] ; NASA through NASA Hubble Fellowship - Space Telescope Science Institute[HST-HF2-51452.001-A] ; NASA[NNX15AB19G] ; NASA[80NSSC20K0523] ; NASA[NAS5-26555] ; ROMFORSK Grant Project[302640] ; European Union's H2020 ERC[DarkGRA-75748] ; Amaldi Research Center - MIUR program Dipartimento di Eccellenza[CUP: B81I18001170001] ; European Union's H2020 ERC Consolidator Grant Binary Massive Black Hole Astrophysics (BMassive)[818691] ; Sloan Foundation Research Fellowship ; Owens Family Foundation ; Science and Technology Facilities Council Ernest Rutherford Fellowship[ST/R003904/1] ; Academy of Finland[324882] ; Academy of Finland[328958] ; GWverse COST Action[CA16104] ; Simons Foundation ; United States National Science Foundation (NSF) ; Science and Technology Facilities Council (STFC) of the United Kingdom ; Max-Planck-Society (MPS) ; State of Niedersachsen/Germany ; Australian Research Council ; European Gravitational Observatory (EGO) ; French Centre National de Recherche Scientifique (CNRS) ; Italian Istituto Nazionale di Fisica Nucleare (INFN) ; Dutch Nikhef ; MIUR PRIN programme (GW-NEXT)[CUP: B84I20000100001] ; MIUR FARE programme (GW-NEXT)[CUP: B84I20000100001] |
| WOS研究方向 | Astronomy & Astrophysics ; Physics |
| 语种 | 英语 |
| WOS记录号 | WOS:000734788400001 |
| 出版者 | SPRINGER/PLENUM PUBLISHERS |
| 源URL | [http://ir.amss.ac.cn/handle/2S8OKBNM/59790]  |
| 专题 | 中国科学院数学与系统科学研究院 |
| 通讯作者 | Blas, Diego |
| 作者单位 | 1.Univ Politecn Valencia, Inst Multidisciplinary Math, Valencia, Spain 2.DESY Zeuthen, Zeuthen, Germany 3.Chinese Acad Sci, Inst Appl Math, Acad Math & Syst Sci, Beijing, Peoples R China 4.Kavli Inst Astron & Astrophys, Beijing, Peoples R China 5.Heidelberg Univ, Astron Rech Inst, Zentrum Astron, Monchofstr 12-14, Heidelberg, Germany 6.Univ Paris, Astroparticule & Cosmol, CNRS, F-75006 Paris, France 7.Moscow Inst Phys & Technol, Dolgoprudnyi, Moscow Region, Russia 8.Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CI, Dept Phys & Astron, 1800 Sherman Ave, Evanston, IL 60201 USA 9.Univ Glasgow, Sch Phys & Astron, SUPA, Kelvin Bldg,Univ Ave, Glasgow G12 8QQ, Lanark, Scotland 10.Johns Hopkins Univ, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA |
| 推荐引用方式 GB/T 7714 | Seoane, Pau Amaro,Sedda, Manuel Arca,Babak, Stanislav,et al. The effect of mission duration on LISA science objectives[J]. GENERAL RELATIVITY AND GRAVITATION,2022,54(1):47. |
| APA | Seoane, Pau Amaro.,Sedda, Manuel Arca.,Babak, Stanislav.,Berry, Christopher P. L..,Berti, Emanuele.,...&Zimmerman, Aaron.(2022).The effect of mission duration on LISA science objectives.GENERAL RELATIVITY AND GRAVITATION,54(1),47. |
| MLA | Seoane, Pau Amaro,et al."The effect of mission duration on LISA science objectives".GENERAL RELATIVITY AND GRAVITATION 54.1(2022):47. |
入库方式： OAI收割
来源：数学与系统科学研究院
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