The Nobel Prize (Swedish pronunciation: [noˈbɛl], Swedish definite form, singular: Nobelpriset, Norwegian: Nobelprisen) is a set of annual international awards bestowed in a number of categories by Scandinavian committees in recognition of cultural and scientific advances. The will of the Swedish chemist Alfred Nobel, the inventor of dynamite, established the prizes in 1895. The prizes in Physics, Chemistry, Physiology or Medicine, Literature, and Peace were first awarded in 1901.

The Peace Prize is awarded in Oslo, Norway, while the other prizes are awarded in Stockholm, Sweden. The Nobel Prize is widely regarded as the most prestigious award available in the fields of literature, medicine, physics, chemistry, peace and economics.

In 1968, Sveriges Riksbank instituted an award that is often associated with the Nobel prizes, the Sveriges Riksbank Prize in Economic Sciences in Memory of Alfred Nobel. The first such prize was awarded in 1969. Although it is not an official Nobel Prize, its announcements and presentations are made along with the other prizes.

Martin Karplus (born March 15, 1930, Vienna) is an Austrian-born American theoretical chemist. He has been Theodore William Richards Professor of Chemistry at Harvard University since 1979. He is also Director of the Biophysical Chemistry Laboratory, a joint laboratory of CNRS and Universite de Strasbourg in Strasbourg, France.

He received a BA degree from Harvard University in 1950, and a Ph.D. from California Institute of Technology in 1953 while working with Linus Pauling. He was an NSF Postdoctoral Fellow at Oxford University (1953–55) where he worked with Charles Coulson. His brother, Robert Karplus, was an internationally recognised physicist and educator at University of California, Berkeley.

Martin Karplus has made significant contributions to many fields in physical chemistry, including the nuclear magnetic resonance spectroscopy, chemical dynamics, quantum chemistry, and most notably, the molecular dynamics simulations of biological macromolecules.

Karplus has made varied contributions to nuclear magnetic resonance spectroscopy, particularly to the understanding of nuclear spin-spin coupling and electron spin resonance spectroscopy. The Karplus equation describing the correlation between coupling constants and dihedral angles in protein nuclear magnetic resonance spectroscopy is named after him.

Brian Greene (born February 9, 1963) is an American theoretical physicist and string theorist. He has been a professor at Columbia University since 1996. Greene has worked on mirror symmetry, relating two different Calabi-Yau manifolds (concretely, relating the conifold to one of its orbifolds). He also described the flop transition, a mild form of topology change, showing that topology in string theory can change at the conifold point. He has become known to a wider audience through his books for the general public, The Elegant Universe, Icarus at the Edge of Time, The Fabric of the Cosmos, The Hidden Reality, and a related PBS television special. Greene also appeared on The Big Bang Theory episode "The Herb Garden Germination."

Greene was born in New York City. His father, Alan Greene, was a one-time vaudeville performer and high school dropout who later worked as a voice coach and composer. After attending Stuyvesant High School, Greene entered Harvard in 1980 to concentrate in physics. After completing his bachelor's degree, Greene earned his doctorate from Oxford University as a Rhodes Scholar, graduating in 1987. While at Oxford, Greene also studied piano with the concert pianist Jack Gibbons.

George Fitzgerald Smoot III (born February 20, 1945) is an American astrophysicist, cosmologist, Nobel laureate, and $1 million TV quiz show prize winner (Are You Smarter Than a 5th Grader?). He won the Nobel Prize in Physics in 2006 for his work on the Cosmic Background Explorer with John C. Mather that led to the measurement "of the black body form and anisotropy of the cosmic microwave background radiation."

This work helped further the Big Bang theory of the universe using the Cosmic Background Explorer Satellite (COBE). According to the Nobel Prize committee, "the COBE project can also be regarded as the starting point for cosmology as a precision science." Smoot donated his share of the Nobel Prize money, less travel costs, to a charitable foundation.

Currently he is a professor of physics at the University of California, Berkeley, senior scientist at the Lawrence Berkeley National Laboratory, and since 2010, a professor of physics at the Paris Diderot University, France. In 2003, he was awarded the Einstein Medal.

Brian P. Schmidt FRS (born February 24, 1967) is a Distinguished Professor, Australian Research Council Laureate Fellow and astrophysicist at The Australian National University Mount Stromlo Observatory and Research School of Astronomy and Astrophysics and is known for his research in using supernovae as cosmological probes. He currently holds an Australia Research Council Federation Fellowship and was elected to the Royal Society in 2012. Schmidt shared both the 2006 Shaw Prize in Astronomy and the 2011 Nobel Prize in Physics with Saul Perlmutter and Adam Riess for providing evidence that the expansion of the universe is accelerating.

Schmidt, an only child, was born on February 24, 1967, in Missoula, Montana, where his father Dana C. Schmidt was a fisheries biologist. When he was 13, his family relocated to Anchorage, Alaska.

Schmidt attended Bartlett High School in Anchorage, Alaska, and graduated in 1985. He has said that he wanted to be a meteorologist "since I was about five-years-old" but "... I did some work at the USA National Weather Service up in Anchorage and didn't enjoy it very much. It was less scientific, not as exciting as I thought it would be—there was a lot of routine. But I guess I was just a little naive about what being a meteorologist meant." His decision to study astronomy, which he had seen as "a minor pastime", was made just before he enrolled at university. He earned his BS (Physics) and BS (Astronomy) from the University of Arizona in 1989. He received his MA (1992) and then PhD from Harvard University in 1993. Schmidt's PhD thesis was supervised by Robert Kirshner and used Type II Supernovae to measure the Hubble Constant.