Freese has contributed to early research on
dark matter and
dark energy. She was one of the first to propose ways to discover dark matter. Her idea of indirect detection in the Earth is being pursued by the
IceCube Neutrino Observatory experiment, and the "wind" of dark matter particles felt as the Earth orbits the
Milky Way (work with
David Spergel) is being searched for in worldwide experiments. Her work decisively ruled out
MACHO (Massive compact halo object) dark matter in favor of
WIMPs (weakly interacting massive particles). She has proposed a model known as "
Cardassian expansion," in which dark energy is replaced with a modification of
Einstein's equations. Recently she proposed a new theoretical type of star, called a
dark star, powered by dark matter annihilation rather than fusion. is a theoretically well-motivated variant of inflation; it uses axionic-type particles to provide the required flat potentials to drive the expansion. In 2013, observations made by the
European Space Agency's
Planck Satellite show that the framework of natural inflation matches the data. This is now strongly disfavoured by the more recent Planck 2018 and BICEP2/Keck data. She has studied the
Ultimate fate of the universe, including the fate of life in the universe. Freese has served on the board of the
Kavli Institute for Theoretical Physics in Santa Barbara and the board of the
Aspen Center for Physics. From 2008 to 2012 she was a councilor and member of the executive committee of the
American Physical Society, She has also served as a member of the board for the
Oskar Klein Centre for Cosmoparticle Physics in Stockholm. == Honors ==