|
Lawrence Schulman
Lawrence S. Schulman (born 1941) is an American-Israeli physicist known for his work on path integrals, quantum measurement theory and statistical mechanics. He introduced topology into path integrals on multiply connected spaces and has contributed to diverse areas from galactic morphology to the arrow of time. Biography He was born to Anna and Louis Schulman in Newark, New Jersey, USA. He first went to the local public school, but switched to more Jewish oriented institutions, graduating from Yeshiva University in 1963. While still in college he married Claire Frangles Sherman. From Yeshiva he went to Princeton where he received the Ph.D. in physics for his thesis (under Arthur Wightman) ''A path integral for spin''. After completing his thesis he took a position as Assistant Professor at Indiana University (Bloomington), but in 1970 went to the Technion-Israel Institute of Technology in Haifa on a NATO postdoctoral fellowship. At the Technion he accepted a position as A ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
United States
The United States of America (U.S.A. or USA), commonly known as the United States (U.S. or US) or America, is a country primarily located in North America. It consists of 50 states, a federal district, five major unincorporated territories, nine Minor Outlying Islands, and 326 Indian reservations. The United States is also in free association with three Pacific Island sovereign states: the Federated States of Micronesia, the Marshall Islands, and the Republic of Palau. It is the world's third-largest country by both land and total area. It shares land borders with Canada to its north and with Mexico to its south and has maritime borders with the Bahamas, Cuba, Russia, and other nations. With a population of over 333 million, it is the most populous country in the Americas and the third most populous in the world. The national capital of the United States is Washington, D.C. and its most populous city and principal financial center is New York City. Paleo-Americ ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Galactic Morphology
Galaxy morphological classification is a system used by astronomers to divide galaxies into groups based on their visual appearance. There are several schemes in use by which galaxies can be classified according to their morphologies, the most famous being the Hubble sequence, devised by Edwin Hubble and later expanded by Gérard de Vaucouleurs and Allan Sandage. However, galaxy classification and morphology are now largely done using computational methods and physical morphology. Hubble sequence The Hubble sequence is a morphological classification scheme for galaxies invented by Edwin Hubble in 1926. It is often known colloquially as the “Hubble tuning-fork” because of the shape in which it is traditionally represented. Hubble's scheme divides galaxies into three broad classes based on their visual appearance (originally on photographic plates): * Elliptical galaxies have smooth, featureless light distributions and appear as ellipses in images. They are denoted by the l ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
