麻豆传媒

Jocelyn Read is an astrophysicist who studies neutron stars 鈥� the remnant cores of dead stars that didn't quite have enough mass to end up as black holes. A leading binary neutron star expert, she focuses on how matter behaves at the extremely high densities inside neutron stars and how this might be measured from astronomical observations of X-rays, gamma-ray bursts and gravitational waves. 

She and her students work to understand and model how neutron stars interact, collide and radiate energy to learn more about their structure and composition. 

Read joined Cal State Fullerton in 2012 and has received numerous grants for her research. Most recently, she was awarded nearly $1 million from the National Science Foundation to lead a project to recruit and support underrepresented students, in particular Latino students, in gravitational-wave science. The grant supports CSUF and Citrus College students engaged in undergraduate research, as well as CSUF alumni in the doctoral program in gravitational-wave astrophysics at Syracuse University.

A native of Calgary, Alberta, Canada, Read earned her doctorate in physics from the University of Wisconsin-Milwaukee and a bachelor's degree in mathematics and physics from the University of British Columbia in Vancouver. She completed postdoctoral work at the Albert Einstein Institute in Germany and at the University of Mississippi. 

Read, a member of the聽LIGO Scientific Collaboration, serves as associate director of CSUF's Gravitational-Wave Physics and Astronomy Center. She is the recipient of the 2017 "Women of the Year" award in聽the category of science and technology from state Sen. Josh Newman.聽

For additional CSUF materials and resources, please visit these websites:
鈥�	CSUF 麻豆传媒 Center: http://news.fullerton.edu
鈥�	CSUF Gravitational-Wave Physics and Astronomy Center: http://physics.fullerton.edu/gwpac/
鈥�	CSUF Scientists Contribute to First Discovery: http://news.fullerton.edu/gravitational-waves/default.aspx

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