LISA double white dwarf binaries as Galactic accelerometers
ORAL
Abstract
*This work was supported by the Argonne National Laboratory under Award No. 2F60042; the Army Research Laboratory MAQP program under Contract No. W911NF-19–2-0181; and the University of Maryland Quantum Technology Center. E.B. and V.S. are supported by NSF Grants No.~AST-2006538, PHY-2207502, PHY-090003 and PHY-20043, by NASA Grants No.~20-LPS20-0011 and~21-ATP21-0010, by the Simons Foundation, and by the John Templeton Foundation Grant~62840. This work was also made possible through the support of Grant 63034 from the John Templeton Foundation. The opinions expressed in this publication are those of the authors and do not necessarily reflect the views of the John Templeton Foundation. E.B. and V.S. acknowledge support from the ITA-USA Science and Technology Cooperation program supported by the Ministry of Foreign Affairs of Italy (MAECI) and from the Indo-US Science and Technology Forum through the Indo-US Centre for Gravitational-Physics and Astronomy, grant~IUSSTF/JC-142/2019. E.H.T. acknowledges support by NSF Grant PHY-2310429 and Gordon and Betty Moore Foundation Grant No. GBMF7946.
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Publication: https://arxiv.org/abs/2405.13109
Presenters
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Reza Ebadi
- University of Maryland College Park