Project Grant 2205974

Award Date 9/1/22
Completion Date 8/31/25
Dollars Obligated $370K
Federal Grant Program
47.049
Assistance Type
Project Grant
Place of Performance
Pasadena, CA 91125, USA
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Through this funding, Caltech researchers will study the formation pathways of binary compact object systems containing black holes and neutron stars. They will use advanced computational modeling techniques to better understand the physical processes governing how these binary systems lose angular momentum over time to enable the two remnants to inspiral and merge. Specific projects include evolutionary calculations of binary white dwarf models, implementing additional angular momentum loss mechanisms in binary stellar evolution models, and modeling light curves from stripped supernovae resulting from binary mass transfer. The research aims to constrain these processes to determine gravitational wave and electromagnetic signatures from compact binary mergers. The grant also supports efforts to retain underrepresented minority students in STEM fields through research opportunities and mentoring.

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