Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q18720091> ?p ?o }
Showing triples 1 to 47 of
47
with 100 triples per page.
- Q18720091 description "physicist".
- Q18720091 description "physicist".
- Q18720091 subject Q3919876.
- Q18720091 subject Q5312304.
- Q18720091 subject Q7453817.
- Q18720091 subject Q8752099.
- Q18720091 abstract "James Lattimer is a nuclear astrophysicist who works on the dense nuclear matter equation of state and neutron stars. He is a Distinguished Professor of Physics and Astronomy at Stony Brook University. He is an American Physical Society Fellow (2001), and has received a Guggenheim (J.S.) Fellowship (1999), a Sloan (Alfred P.) Fellowship (1982), and the Fullam (Ernest F.) Award from Dudley Observatory (1985). In 2015, Lattimer was awarded the Hans Bethe Prize for "outstanding theoretical work connecting observations of supernovae and neutron stars with neutrino emission and the equation of state of matter beyond nuclear density."Lattimer has made a number of fundamental contributions to the field ofnuclear astrophysics, with a particular focus on neutron stars. Oneof his biggest impacts was modeling the birth of neutron stars fromsupernovae in 1986 with then-research assistant professor Adam Burrows. This came just six monthsbefore the closest supernova in modern history (SN 1987A, in theLMC). Their paper predicted the signature of neutrinos fromsupernovae that was subsequently validated by neutrino observations,from SN 1987A on Feb. 23, 1987.In work that led to his PhD thesis, Lattimer and his advisor David N. Schramm firstargued that the mergers of neutron stars and black holes would result in the ejection of neutron-rich matter in sufficient quantities to explain the origin of r-process elements such as gold and platinum. Later, with collaborators, he demonstrated decompressing neutron-star matter from both neutron star-black hole and neutron star-neutron star mergers would form a natural r-process that would match observed patterns.More recently, Lattimer and collaborators suggested thatthe recently observed rapid cooling of the neutron star in theCassiopeia A supernova remnant is the first direct evidence for superfluidity and superconductivityin neutron star interiors.".
- Q18720091 birthDate "1950".
- Q18720091 birthYear "1950".
- Q18720091 wikiPageExternalLink lattimer.
- Q18720091 wikiPageWikiLink Q106667.
- Q18720091 wikiPageWikiLink Q124131.
- Q18720091 wikiPageWikiLink Q1576704.
- Q18720091 wikiPageWikiLink Q17305586.
- Q18720091 wikiPageWikiLink Q207436.
- Q18720091 wikiPageWikiLink Q2126.
- Q18720091 wikiPageWikiLink Q260040.
- Q18720091 wikiPageWikiLink Q285033.
- Q18720091 wikiPageWikiLink Q3919876.
- Q18720091 wikiPageWikiLink Q3937.
- Q18720091 wikiPageWikiLink Q4202.
- Q18720091 wikiPageWikiLink Q5312304.
- Q18720091 wikiPageWikiLink Q589.
- Q18720091 wikiPageWikiLink Q618273.
- Q18720091 wikiPageWikiLink Q6579918.
- Q18720091 wikiPageWikiLink Q7068141.
- Q18720091 wikiPageWikiLink Q7453817.
- Q18720091 wikiPageWikiLink Q8752099.
- Q18720091 wikiPageWikiLink Q969850.
- Q18720091 dateOfBirth "1950".
- Q18720091 name "Lattimer, James M.".
- Q18720091 shortDescription "physicist".
- Q18720091 type Person.
- Q18720091 type Agent.
- Q18720091 type Person.
- Q18720091 type Agent.
- Q18720091 type NaturalPerson.
- Q18720091 type Thing.
- Q18720091 type Q215627.
- Q18720091 type Q5.
- Q18720091 type Person.
- Q18720091 comment "James Lattimer is a nuclear astrophysicist who works on the dense nuclear matter equation of state and neutron stars. He is a Distinguished Professor of Physics and Astronomy at Stony Brook University. He is an American Physical Society Fellow (2001), and has received a Guggenheim (J.S.) Fellowship (1999), a Sloan (Alfred P.) Fellowship (1982), and the Fullam (Ernest F.) Award from Dudley Observatory (1985).".
- Q18720091 label "James Lattimer".
- Q18720091 givenName "James M.".
- Q18720091 name "James M. Lattimer".
- Q18720091 name "Lattimer, James M.".
- Q18720091 surname "Lattimer".