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Famous Physicists Himansu Sekhar Fatesingh
Fun Quiz FAMOUS PHYSICISTS HIMANSU SEKHAR FATESINGH 1. The first woman to 6. He first succeeded in receive the Nobel Prize in producing the nuclear physics was chain reaction. a. Maria G. Mayer a. Otto Hahn b. Irene Curie b. Fritz Strassmann c. Marie Curie c. Robert Oppenheimer d. Lise Meitner d. Enrico Fermi 2. Who first suggested electron 7. The credit for discovering shells around the nucleus? electron microscope is often a. Ernest Rutherford attributed to b. Neils Bohr a. H. Germer c. Erwin Schrödinger b. Ernst Ruska d. Wolfgang Pauli c. George P. Thomson d. Clinton J. Davisson 8. The wave theory of light was 3. He first measured negative first proposed by charge on an electron. a. Christiaan Huygens a. J. J. Thomson b. Isaac Newton b. Clinton Davisson c. Hermann Helmholtz c. Louis de Broglie d. Augustin Fresnel d. Robert A. Millikan 9. He was the first scientist 4. The existence of quarks was to find proof of Einstein’s first suggested by theory of relativity a. Max Planck a. Edwin Hubble b. Sheldon Glasgow b. George Gamow c. Murray Gell-Mann c. S. Chandrasekhar d. Albert Einstein d. Arthur Eddington 10. The credit for development of the cyclotron 5. The phenomenon of goes to: superconductivity was a. Carl Anderson b. Donald Glaser discovered by c. Ernest O. Lawrence d. Charles Wilson a. Heike Kamerlingh Onnes b. Alex Muller c. Brian D. Josephson 11. Who first proposed the use of absolute scale d. John Bardeen of Temperature? a. Anders Celsius b. Lord Kelvin c. Rudolf Clausius d. -
Catholic Christian Christian
Religious Scientists (From the Vatican Observatory Website) https://www.vofoundation.org/faith-and-science/religious-scientists/ Many scientists are religious people—men and women of faith—believers in God. This section features some of the religious scientists who appear in different entries on these Faith and Science pages. Some of these scientists are well-known, others less so. Many are Catholic, many are not. Most are Christian, but some are not. Some of these scientists of faith have lived saintly lives. Many scientists who are faith-full tend to describe science as an effort to understand the works of God and thus to grow closer to God. Quite a few describe their work in science almost as a duty they have to seek to improve the lives of their fellow human beings through greater understanding of the world around them. But the people featured here are featured because they are scientists, not because they are saints (even when they are, in fact, saints). Scientists tend to be creative, independent-minded and confident of their ideas. We also maintain a longer listing of scientists of faith who may or may not be discussed on these Faith and Science pages—click here for that listing. Agnesi, Maria Gaetana (1718-1799) Catholic Christian A child prodigy who obtained education and acclaim for her abilities in math and physics, as well as support from Pope Benedict XIV, Agnesi would write an early calculus textbook. She later abandoned her work in mathematics and physics and chose a life of service to those in need. Click here for Vatican Observatory Faith and Science entries about Maria Gaetana Agnesi. -
The Schwarzschild Metric and Applications 1
The Schwarzschild Metric and Applications 1 Analytic solutions of Einstein's equations are hard to come by. It's easier in situations that e hibit symmetries. 1916: Karl Schwarzschild sought the metric describing the static, spherically symmetric spacetime surrounding a spherically symmetric mass distribution. A static spacetime is one for which there exists a time coordinate t such that i' all the components of g are independent of t ii' the line element ds( is invariant under the transformation t -t A spacetime that satis+es (i) but not (ii' is called stationary. An example is a rotating azimuthally symmetric mass distribution. The metric for a static spacetime has the form where xi are the spatial coordinates and dl( is a time*independent spatial metric. -ross-terms dt dxi are missing because their presence would violate condition (ii'. 23ote: The Kerr metric, which describes the spacetime outside a rotating ( axisymmetric mass distribution, contains a term ∝ dt d.] To preser)e spherical symmetry& dl( can be distorted from the flat-space metric only in the radial direction. In 5at space, (1) r is the distance from the origin and (2) 6r( is the area of a sphere. Let's de+ne r such that (2) remains true but (1) can be violated. Then, A,xi' A,r) in cases of spherical symmetry. The Ricci tensor for this metric is diagonal, with components S/ 10.1 /rimes denote differentiation with respect to r. The region outside the spherically symmetric mass distribution is empty. 9 The vacuum Einstein equations are R = 0. To find A,r' and B,r'# (. -
J. Robert Schrieffer Strange Quantum Numbers in Condensed Matter
Wednesday, May 1, 2002 3:00 pm APS Auditorium, Building 402, Argonne National Laboratory APS Colloquium home J. Robert Schrieffer Nobel Laureate National High Magnetic Field Laboratory Florida State University, Tallahassee [email protected] http://www.physics.fsu.edu/research/NHMFL.htm Strange Quantum Numbers in Condensed Matter Physics The origin of peculiar quantum numbers in condensed matter physics will be reviewed. The source of spin-charge separation and fractional charge in conducting polymers has to do with solitons in broken symmetry states. For superconductors with an energy gap, which is odd under time reversal, reverse spin-orbital angular momentum pairing occurs. In the fractional quantum Hall effect, quasi particles of fractional charge occur. In superfluid helium 3, a one-way branch of excitations exists if a domain wall occurs in the system. Many of these phenomena occur due to vacuum flow of particles without crossing the excitation of the energy gap. John Robert Schrieffer received his bachelor's degree from Massachusetts Institute of Technology in 1953 and his Ph.D. from the University of Illinois in 1957. In addition, he holds honorary Doctor of Science degrees from universities in Germany, Switzerland, and Israel, and from the University of Pennsylvania, the University of Cincinnati, and the University of Alabama. Since 1992, Dr. Schrieffer has been a professor of Physics at Florida State University and the University of Florida and the Chief Scientist of the National High Magnetic Field Laboratory. He also holds the FSU Eminent Scholar Chair in Physics. Before moving to Florida in 1991, he served as director for the Institute for Theoretical Physics from 1984-1989 and was the Chancellor's Professor at the University of California in Santa Barbara from 1984-1991. -
Samuel Goudsmit
NATIONAL ACADEMY OF SCIENCES SAMUEL ABRAHAM GOUDSMIT 1 9 0 2 — 1 9 7 8 A Biographical Memoir by BENJAMIN BEDERSON Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 2008 NATIONAL ACADEMY OF SCIENCES WASHINGTON, D.C. Photograph courtesy Brookhaven National Laboratory. SAMUEL ABRAHAM GOUDSMIT July 11, 1902–December 4, 1978 BY BENJAMIN BEDERSON AM GOUDSMIT LED A CAREER that touched many aspects of S20th-century physics and its impact on society. He started his professional life in Holland during the earliest days of quantum mechanics as a student of Paul Ehrenfest. In 1925 together with his fellow graduate student George Uhlenbeck he postulated that in addition to mass and charge the electron possessed a further intrinsic property, internal angular mo- mentum, that is, spin. This inspiration furnished the missing link that explained the existence of multiple spectroscopic lines in atomic spectra, resulting in the final triumph of the then struggling birth of quantum mechanics. In 1927 he and Uhlenbeck together moved to the United States where they continued their physics careers until death. In a rough way Goudsmit’s career can be divided into several separate parts: first in Holland, strictly as a theorist, where he achieved very early success, and then at the University of Michigan, where he worked in the thriving field of preci- sion spectroscopy, concerning himself with the influence of nuclear magnetism on atomic spectra. In 1944 he became the scientific leader of the Alsos Mission, whose aim was to determine the progress Germans had made in the development of nuclear weapons during World War II. -
Almanac, 03/28/78, Vol. 24, No. 25
Lniphnee Pertormance Review Of Record: Office of ('o#nputinç' Activities Photocop ring for Educational Uses Published the of Weekly by University Pennsylvania Report of the Provost's Task Force on the Study of Ad,,,:ssions Volume 24, Number 25 March 28, 1978 Annenberg Friends Contribute Funds, Support The Annenherg Preservation Committee, a student organi/ation headed by undergraduate Ray (Ireenherg, and the Friends of the Zellerhach Theater are helping the Annenherg Center meet its $125.000 fundraising goal and ensure the continuance of a professional theater season here next year. Approximately $500 collected by the Annenherg Preservation Committee during the student sit-in March 2-6 which was in part sparked h' the proposal to limit or curtail professional theater at Annenherg was presented to Annenhcrg Center Managing Director Stephen Goff last week. The committee is now offering for sale "Save the Center" t-shirts ($3) and buttons ($I). One dollar from every sale will go to the Annenberg Center. The committee is also arranging a special Penn All-Star Revue performance in May to benefit the Center. Another group. Friends of the Zellerhach Theater, headed by Diana Dripps and trustee Robert Trescher, will sponsor a gala benefit performance of Much Ado About Nothing, which they are Book fro,n the University of Pennsylvania Press edition of calling "Much Ado About Something." Seats will sell for $50 and jacket The Gentleman. $100. and anonymous donors have agreed to match funds raised Country from the special event. "Lost" Comedy to Premiere In addition, all funds raised by both groups will he applicable to a A Country Gentleman, a comedy written and banned n 1669 and challenge grant which may be awarded by the National Endowment considered lost for more than 3(X) years will hac its world for the Arts. -
Wolfgang Pauli Niels Bohr Paul Dirac Max Planck Richard Feynman
Wolfgang Pauli Niels Bohr Paul Dirac Max Planck Richard Feynman Louis de Broglie Norman Ramsey Willis Lamb Otto Stern Werner Heisenberg Walther Gerlach Ernest Rutherford Satyendranath Bose Max Born Erwin Schrödinger Eugene Wigner Arnold Sommerfeld Julian Schwinger David Bohm Enrico Fermi Albert Einstein Where discovery meets practice Center for Integrated Quantum Science and Technology IQ ST in Baden-Württemberg . Introduction “But I do not wish to be forced into abandoning strict These two quotes by Albert Einstein not only express his well more securely, develop new types of computer or construct highly causality without having defended it quite differently known aversion to quantum theory, they also come from two quite accurate measuring equipment. than I have so far. The idea that an electron exposed to a different periods of his life. The first is from a letter dated 19 April Thus quantum theory extends beyond the field of physics into other 1924 to Max Born regarding the latter’s statistical interpretation of areas, e.g. mathematics, engineering, chemistry, and even biology. beam freely chooses the moment and direction in which quantum mechanics. The second is from Einstein’s last lecture as Let us look at a few examples which illustrate this. The field of crypt it wants to move is unbearable to me. If that is the case, part of a series of classes by the American physicist John Archibald ography uses number theory, which constitutes a subdiscipline of then I would rather be a cobbler or a casino employee Wheeler in 1954 at Princeton. pure mathematics. Producing a quantum computer with new types than a physicist.” The realization that, in the quantum world, objects only exist when of gates on the basis of the superposition principle from quantum they are measured – and this is what is behind the moon/mouse mechanics requires the involvement of engineering. -
Ernest Rutherford and the Accelerator: “A Million Volts in a Soapbox”
Ernest Rutherford and the Accelerator: “A Million Volts in a Soapbox” AAPT 2011 Winter Meeting Jacksonville, FL January 10, 2011 H. Frederick Dylla American Institute of Physics Steven T. Corneliussen Jefferson Lab Outline • Rutherford's call for inventing accelerators ("million volts in a soap box") • Newton, Franklin and Jefferson: Notable prefiguring of Rutherford's call • Rutherfords's discovery: The atomic nucleus and a new experimental method (scattering) • A century of particle accelerators AAPT Winter Meeting January 10, 2011 Rutherford’s call for inventing accelerators 1911 – Rutherford discovered the atom’s nucleus • Revolutionized study of the submicroscopic realm • Established method of making inferences from particle scattering 1927 – Anniversary Address of the President of the Royal Society • Expressed a long-standing “ambition to have available for study a copious supply of atoms and electrons which have an individual energy far transcending that of the alpha and beta particles” available from natural sources so as to “open up an extraordinarily interesting field of investigation.” AAPT Winter Meeting January 10, 2011 Rutherford’s wish: “A million volts in a soapbox” Spurred the invention of the particle accelerator, leading to: • Rich fundamental understanding of matter • Rich understanding of astrophysical phenomena • Extraordinary range of particle-accelerator technologies and applications AAPT Winter Meeting January 10, 2011 From Newton, Jefferson & Franklin to Rutherford’s call for inventing accelerators Isaac Newton, 1717, foreseeing something like quarks and the nuclear strong force: “There are agents in Nature able to make the particles of bodies stick together by very strong attractions. And it is the business of Experimental Philosophy to find them out. -
Copyrighted Material
The Composition of Matter 1 “Everything existing in the universe is the fruit of chance and necessity.” —Democritus 1.1 EARLY DESCRIPTIONS OF MATTER Chemistry has been defined as the study of matter and its interconversions. Thus, ina sense, chemistry is a study of the physical world in which we live. But how much do we really know about the fundamental structure of matter and its relationship to the larger macroscopic world? I have in my rock collection, which I have had since I was a boy, a sample of the mineral cinnabar, which is several centimeters across and weighs about 10 g. Cinnabar is a reddish granular solid with a density about eight times that of water and the chemical composition mercuric sulfide. Now suppose that some primal instinct suddenly overcame me and I were inclined to demolish this precious talisman from my childhood. I could take a hammer to it and smash it into a billion little pieces. Choosing the smallest of these chunks, I could further disintegrate the material in a mortar and pestle, grinding it into ever finer and finer grains until Iwas left with nothing but a red powder (in fact, this powder is known as vermilion and has been used as a red pigment in artwork dating back to the fourteenth century). Having satisfied my destructive tendencies, I would nonetheless still have exactly the same material that I started with—that is, it would have precisely the same chemical and physical properties as the original. I might therefore wonder to myself if there is some inherent limitation as to how finely I can divide the substance or if this is simply limited by the tools at my disposal. -
Twenty Five Hundred Years of Small Science What’S Next?
Twenty Five Hundred Years of Small Science What’s Next? Lloyd Whitman Assistant Director for Nanotechnology White House Office of Science and Technology Policy Workshop on Integrated Nanosystems for Atomically Precise Manufacturing Berkeley, CA, August 5, 2015 Democritus (ca. 460 – 370 BC) Everything is composed of “atoms” Atomos (ἄτομος): that which can not be cut www.phil-fak.uni- duesseldorf.de/philo/galerie/antike/ demokrit.html Quantum Mechanics (1920s) Max Planck 1918* Albert Einstein 1921 Niels Bohr 1922 Louis de Broglie 1929 Max Born 1954 Paul Dirac 1933 On the Theory of Quanta Louis-Victor de Broglie Werner Heisenberg 1932 Wolfgang Pauli 1945 Erwin Schrödinger 1933 *Nobel Prizes in Physics https://tel.archives-ouvertes.fr/tel- 00006807 Ernst Ruska (1906 – 1988) Electron Microscopy Magnifying higher than the light microscope - 1933 Nobel Prize in Physics 1986 www.nobelprize.org/nobel_prizes/physics/laureates /1986/ruska-lecture.pdf Richard Feynman (1918-1988) There's Plenty of Room at the Bottom, An Invitation to Enter a New Field of Physics What would happen if we could arrange the atoms one by one the way we want them…? December 29, 1959 richard-feynman.net Heinrich Rohrer (1933 – 2013) Gerd Binnig Atomic resolution Scanning Tunneling Microscopy - 1981 1983 I could not stop looking at the images. It was like entering a new world. Gerd Binnig, Nobel lecture Binnig, et al., PRL 50, 120 (1983) Nobel Prize in Physics 1986 C60: Buckminsterfullerene Kroto, Heath, O‘Brien, Curl and September 1985 Smalley - 1985 …a remarkably stable cluster consisting of 60 carbon atoms…a truncated icosahedron. Nature 318, 162 (1985) http://www.acs.org/content/acs/en/education/whatis chemistry/landmarks/fullerenes.html Nobel Prize in Chemistry 1996 Curl, Kroto, and Smalley Positioning Single Atoms with a Scanning Tunnelling Microscope Eigler and Schweizer - 1990 …fabricate rudimentary structures of our own design, atom by atom. -
Appendix E • Nobel Prizes
Appendix E • Nobel Prizes All Nobel Prizes in physics are listed (and marked with a P), as well as relevant Nobel Prizes in Chemistry (C). The key dates for some of the scientific work are supplied; they often antedate the prize considerably. 1901 (P) Wilhelm Roentgen for discovering x-rays (1895). 1902 (P) Hendrik A. Lorentz for predicting the Zeeman effect and Pieter Zeeman for discovering the Zeeman effect, the splitting of spectral lines in magnetic fields. 1903 (P) Antoine-Henri Becquerel for discovering radioactivity (1896) and Pierre and Marie Curie for studying radioactivity. 1904 (P) Lord Rayleigh for studying the density of gases and discovering argon. (C) William Ramsay for discovering the inert gas elements helium, neon, xenon, and krypton, and placing them in the periodic table. 1905 (P) Philipp Lenard for studying cathode rays, electrons (1898–1899). 1906 (P) J. J. Thomson for studying electrical discharge through gases and discover- ing the electron (1897). 1907 (P) Albert A. Michelson for inventing optical instruments and measuring the speed of light (1880s). 1908 (P) Gabriel Lippmann for making the first color photographic plate, using inter- ference methods (1891). (C) Ernest Rutherford for discovering that atoms can be broken apart by alpha rays and for studying radioactivity. 1909 (P) Guglielmo Marconi and Carl Ferdinand Braun for developing wireless telegraphy. 1910 (P) Johannes D. van der Waals for studying the equation of state for gases and liquids (1881). 1911 (P) Wilhelm Wien for discovering Wien’s law giving the peak of a blackbody spectrum (1893). (C) Marie Curie for discovering radium and polonium (1898) and isolating radium. -
Melvin Schwartz 1932-2006
MELVIN SCHWARTZ 1932-2006 A Biographical Memoir by N. P. SAMIOS AND P. YAMIN © 2012 The National Academy of Sciences Any opinions expressed in this memoir are those of the authors and do not necessarily reflect the views of the National Academy of Sciences. MELVIN SCHWARTZ Courtesy of Brookhaven National Laboratories. November 2, 1932–August 28, 2006 BY N. P. SAMIOS AND P. YAMIN MEL SCHWARTZ DIED ON August 28, 2006, in Twin Falls, Idaho. He was born on 1 November 2, 1932, in New York City. He grew up in the Great Depression, but with a sense of optimism and desire to use his mind for the betterment of human- kind. He entered the Bronx High School of Science in the fall of 1945. It was there that his interest in physics began and that he recognized the importance of interactions with peers in determining his sense of direction in life. One of his classmates and future colleagues recalled that “even then” he wanted a Nobel Prize. Mel noted: My interest in physics began at the age of 12 when I entered the Bronx High School of Science. The four years I spent there were certainly among the most exciting and stimulating in my life, mostly because of the interaction with the other students of similar background, interest, and ability. MELVIN SCHWARTZ MELVIN On Sunday afternoons he attended a school run by the secular and Zionist Yiddish and many others. As Mel commented, “This faculty [was] at this time unmatched by any in the world, largely Nationaler Arbeter Farband (Jewish National Workers Alliance).