Multimessenger Science Opportunities with mHz Gravitational Waves

Baker, John ; Haiman, Zoltan ; Rossi, Elena Maria ; Berger, Edo ; Brandt, Niel ; Breedt, Elme ; Breivik, Katelyn ; Charisi, Maria ; Derdzinski, Andrea ; D’Orazio, Daniel J(Harvard Univ, Cambridge, MA, United States)

关键词: ASTROPHYSICS;    BLACK HOLES (ASTRONOMY);    GALACTIC EVOLUTION;    GRAVITATION;    GRAVITATIONAL WAVES;    MILKY WAY GALAXY;    OBSERVATORIES;    POPULATIONS;    SPECTRA;    GALAXIES;   

RP-ID  :  GSFC-E-DAA-TN66947

学科分类：天体物理学

美国|英语

来源: NASA Technical Reports Server

【 摘 要 】

LISA will open the mHz band of gravitational waves (GWs) to the astronomy community. Thestrong gravity which powers the variety of GW sources in this band is also crucial in a numberof important astrophysical processes at the current frontiers of astronomy. These range fromthe beginning of structure formation in the early universe, through the origin and cosmic evolutionof massive black holes in concert with their galactic environments, to the evolution ofstellar remnant binaries in the Milky Way and in nearby galaxies. These processes and theirassociated populations also drive current and future observations across the electromagnetic(EM) spectrum. We review opportunities for science breakthroughs, involving either direct coincidentEM+GW observations, or indirect multimessenger studies. We argue that for the UScommunity to fully capitalize on the opportunities from the LISA mission, the US efforts shouldbe accompanied by a coordinated and sustained program of multi-disciplinary science investment,following the GW data through to its impact on broad areas of astrophysics. Supportfor LISA-related multimessenger observers and theorists should be sized appropriately for aflagship observatory and may be coordinated through a dedicated mHz GW research center.