Saul Perlmutter (born September 22, 1959) is an American astrophysicist who is a professor of physics at the University of California, Berkeley.
Facts
Birth YearSourced to the subject's own account Birth DateSourced to the subject's own account BirthplaceChampaign, United States 1 Field
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Member Of
Source Saul Perlmutter (Wikipedia)
Source Saul Perlmutter (Wikipedia)
Source Saul Perlmutter (Wikipedia)
Proposed
Additional Source Dark Energy (Wikipedia)Late-time dark energy section (edge: proposed-by, Perlmutter)
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Source Saul Perlmutter (Wikipedia)
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Also in Geography Atlas: the nationality of this subject.
Source Saul Perlmutter (Wikidata)
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1. Saul Perlmutter (Wikidata)
P27 (country of citizenship): United States
Q30
P19 (place of birth): Champaign, United States
Q577964
View the Source2. Saul Perlmutter (Wikipedia)
WikipediaLead section (entity-description)
Saul Perlmutter (born September 22, 1959) is an American astrophysicist who is a professor of physics at the University of California, Berkeley.
Infobox (birth-date)
Born: September 22, 1959
Infobox (birth-year)
Born: September 22, 1959
Works In: Astrophysics, Lead sentence
Saul Perlmutter (born September 22, 1959) is an American astrophysicist who is a professor of physics at the University of California, Berkeley, where he holds the Franklin W. and Karen Weber Dabby Chair, and is head of the International Supernova Cosmology Project at the Lawrence Berkeley National
Member Of: National Academy of Sciences, Article text
He is a member of the National Academy of Sciences. Perlmutter shared the 2006 Shaw Prize
Member Of: American Physical Society, Categories
Category:Fellows of the American Physical Society
Member Of: American Association for the Advancement of Science, Article text
He is a member of both the American Academy of Arts & Sciences and the American Philosophical Society, and was elected a Fellow of the American Association for the Advancement of Science in 2003. He is a member of the Nationa
View the Source Dark Energy (Wikipedia)
WikipediaProposed: Dark Energy, Late-time dark energy section (edge: proposed-by, Perlmutter)Quote, Proposed: Dark Energy, Late-time dark energy section (edge: proposed-by, Perlmutter)
The first direct evidence for dark energy came from supernova observations in 1998 of accelerated expansion in Riess et al. and in Perlmutter et al.
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