THE HIGHLANDER
UNIVERSITY OF CALIFORNIA, RIVERSIDE
est. 1954
FOR THE WEEK OF TUESDAY, SEPTEMBER 25 , 2018
VOL. 67, ISSUE 01
UCR welcomes Nobel prize winner Barry C. Barish
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KARLA URIOSTEGUI Contributing Writer
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In an “America’s Best Colleges Report” by the U.S. News and World Report (USNWR), UC Riverside made larger gains than any other university in the United States. The report factors in graduates’ successful outcomes, social mobility and diversity to rank institutions across the United States.
UC Riverside has signalled its ambition in expanding its awardwinning faculty by hiring the 2017 Physics Nobel Prize winner, Barry C. Barish. On Sept. 1, Barish joined the UCR College of Natural and Agricultural Sciences (CNAS) faculty for the 2018 fall quarter. Barish earned the Prize alongside Rainer Weiss, a professor at the Massachusetts Institute of Technology (MIT), and Kip Thorne, a professor at Caltech University, for their groundbreaking work in enabling the first observation of gravitational waves. Barish and his peers made great contributions in the Laser Interferometer Gravitational Wave Observatory, otherwise known as LIGO. On September 14, 2015, LIGO was able to detect a gravitational wave for the first time ever. The detection of gravitational waves confirms predictions made by Albert Einstein in his general theory of relativity. The LIGO lab contains a total of 1000 researchers from more than 20 countries and enables the detection of gravitational waves caused by different universal phenomena. The first gravitational wave detected was generated by the collision of two black holes and took about 1.3 billion years to arrive at the LIGO detector labs. LIGO allows the detection of gravitational waves by splitting a laser beam with a mirror into two and sends each beam in different directions with a precise time and equal distance through long vacuum tubes. Mirrors located at the end of each tube reflect the lasers back at the same time. When no disturbance is detected, the laser reflections meet and cancel each other out, preventing light from reaching the detecting instruments. ► SEE BARISH PAGE 4
► SEE RANKING PAGE 4
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