Astrophysical observations of a dark matter-baryon fifth force
ORAL
Abstract
Due to intensive theoretical and experimental study over the past several decades, fifth forces between baryonic matter are tightly constrained. Long-range fifth forces between baryonic matter and dark matter are less well studied and constrained. In this talk, I will discuss limits on a long-range force between baryonic and dark matter, focusing in particular on limits from neutron star temperature and pulsar timing observations.
*Some of the work presented was performed at the Aspen Center for Physics, which is supported by National Science Foundation grant PHY-1607611, and some of the presenter's work was supported by the National Science Foundation under Grant No. 1719780.
–
Publication: M.I. Gresham, V.S.H. Lee and K.M. Zurek,
``Astrophysical observations of a dark matter-Baryon fifth force,''
JCAP 02, 048 (2023),
doi:10.1088/1475-7516/2023/02/048,
[arXiv:2209.03963 [astro-ph.HE]].
Presenters
-
Moira I Gresham
- Whitman College