McLaughlin's main research interests involve studying neutron stars and their environments through radio, X-ray and gamma-ray observations. Neutron stars are amazing physical laboratories for general relativity, studies of the interstellar medium, high-energy particle and plasma physics, and studies of stellar evolution. A significant research aim as a member of the NANOGrav collaboration, is to use neutron stars to detect gravitational waves through timing an array of ultra-precise millisecond pulsars. She served as chair and co-director of the NANOGrav Physics Frontiers Center and is also PI on an NSF IRES award which provides students with research experience through the International Pulsar Timing Array collaboration. Her work with the Pulsar Search Collaboratory involves West Virginia high school students in her research. She has been awarded an Alfred P. Sloan Fellowship and a Cottrell Scholar Award from the Research Corporation for her work. Education: B.S. Pennsylvania State University, 1994 Ph.D. Cornell University, 2001
Maura McLaughlin has been named a 2020 Highly Cited Researcher by Web of Science, one of the world鈥檚 top research awards.
19-Jan-2021 09:45:32 AM EST
鈥淭here is a lot of evidence for hierarchical galaxy growth over cosmic time, whereby galaxies grow larger and more structured through mergers. However, there are many unanswered questions about this merger process. How many galaxies are the product of a merger? What are the roles of astrophysical processes such as stellar scattering and accretion in the merger process? By measuring the amplitude and spectrum of the gravitational wave background,鈥 she concluded, 鈥渨e can place important constraints on these questions.鈥
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