Gordon Baym

Gordon Baym

Gordon Alan Baym (born July 1, 1935) is an American theoretical physicist.

Born in New York City, he graduated from the Brooklyn Technical High School, and received his undergraduate degree from Cornell University in 1956. He earned his Ph.D. from Harvard University in 1960, studying under Julian Schwinger.

He joined the physics faculty of the University of Illinois at Urbana-Champaign in 1963, becoming a full professor in 1968. His areas of research range from condensed-matter physics to nuclear physics and astrophysics, as well as the history of physics.

In 1962 he and Leo Kadanoff collaborated on Quantum Statistical Mechanics: Green's Function Methods in Equilibrium and Nonequilibrium Problems. In 1969 he published Lectures on Quantum Mechanics, a widely used graduate textbook that, unconventionally, begins with photon polarization. In 1991 he and Chris Pethick published the monograph Landau Fermi-Liquid Theory: Concepts and Applications.

Baym was awarded the Hans A. Bethe Prize in 2002 "For his superb synthesis of fundamental concepts which have provided an understanding of matter at extreme conditions, ranging from crusts and interiors of neutron stars to matter at ultrahigh temperature".[1] He also received the Lars Onsager Prize in 2008 "for fundamental applications of statistical physics to quantum fluids, including Fermi liquid theory and ground-state properties of dilute quantum gases, and for bringing a conceptual unity to these areas"[2] along with Christopher Pethick and Tin-Lun Ho.

He has four children, professors of communications Nancy Baym and Geoffrey Baym, mathematician and biologist Michael Baym, and cognitive neuroscientist Carol Baym. He was married to Lillian Hoddeson, a professor of History at UIUC.

Awards and honors

References

External links


Wikimedia Foundation. 2010.

Игры ⚽ Поможем решить контрольную работу

Look at other dictionaries:

  • Gordon Baym — Gordon Alan Baym (* 1. Juli 1935 in New York City) ist ein US amerikanischer theoretischer Physiker. Leben und Wirken Baym studierte an der Cornell University (Bachelor 1957) und an der Harvard University Physik und Mathematik (Master Abschluss… …   Deutsch Wikipedia

  • Baym — Gordon A. Baym (* 1. Juli 1935 in New York City) ist ein US amerikanischer theoretischer Physiker. Leben und Wirken Baym studierte an der Cornell University (Bachelor 1957) und an der Harvard University Physik und Mathematik (Master Abschluss in… …   Deutsch Wikipedia

  • Nina Baym — (born 1936)[1] is an American literary critic and literary historian. She was professor of English at the University of Illinois, Urbana Champaign between 1963 and 2004. Before her retirement at the University of Illinois Baym was a Swanlund… …   Wikipedia

  • Lillian Hoddeson — (* 1940 in New York City)[1] ist eine US amerikanische Wissenschaftshistorikerin vor allem der Physik der zweiten Hälfte des 20. Jahrhunderts. Hoddeson besuchte die Bronx High School of Science (Abschluss 1957), studierte Physik am Barnard… …   Deutsch Wikipedia

  • J. Schwinger — Julian Seymour Schwinger, 1965 Julian Seymour Schwinger (* 12. Februar 1918 in New York; † 16. Juli 1994 in Los Angeles) war einer der führenden US amerikanischen theoretischen Physiker. Zusammen mit Richard P. Feynman und …   Deutsch Wikipedia

  • Julian Schwinger — Julian Seymour Schwinger, 1965 Julian Seymour Schwinger (* 12. Februar 1918 in New York; † 16. Juli 1994 in Los Angeles) war einer der führenden US amerikanischen theoretischen Physiker. Zusammen mit Richard P. Feynman und …   Deutsch Wikipedia

  • Liste der Biografien/Bax–Baz — Biografien: A B C D E F G H I J K L M N O P Q …   Deutsch Wikipedia

  • Etoile a neutrons — Étoile à neutrons RX J1856.4 3754, une étoile à neutrons isolée proche du Système solaire, dont l émission de surface est vue par le télescope spatial Hubble. Une étoile à neutrons est le nom donné à un astre principalement composé de neutrons… …   Wikipédia en Français

  • Étoile à neutron — Étoile à neutrons RX J1856.4 3754, une étoile à neutrons isolée proche du Système solaire, dont l émission de surface est vue par le télescope spatial Hubble. Une étoile à neutrons est le nom donné à un astre principalement composé de neutrons… …   Wikipédia en Français

  • Étoile à neutrons — RX J1856.4 3754, une étoile à neutrons isolée proche du Système solaire, dont l émission de surface est vue par le télescope spatial Hubble. Une étoile à neutrons est le nom donné à un astre principalement composé de neutrons maintenus ensemble… …   Wikipédia en Français

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”