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Comments on the 2011 Shaw Prize in Mathematical Sciences - - an Analysis of Collectively Formed Errors in Physics by C
Global Journal of Science Frontier Research Physics and Space Science Volume 12 Issue 4 Version 1.0 June 2012 Type : Double Blind Peer Reviewed International Research Journal Publisher: Global Journals Inc. (USA) Online ISSN: 2249-4626 & Print ISSN: 0975-5896 Comments on the 2011 Shaw Prize in Mathematical Sciences - - An Analysis of Collectively Formed Errors in Physics By C. Y. Lo Applied and Pure Research Institute, Nashua, NH Abstract - The 2011 Shaw Prize in mathematical sciences is shared by Richard S. Hamilton and D. Christodoulou. However, the work of Christodoulou on general relativity is based on obscure errors that implicitly assumed essentially what is to be proved, and thus gives misleading results. The problem of Einstein’s equation was discovered by Gullstrand of the 1921 Nobel Committee. In 1955, Gullstrand is proven correct. The fundamental errors of Christodoulou were due to his failure to distinguish the difference between mathematics and physics. His subsequent errors in mathematics and physics were accepted since judgments were based not on scientific evidence as Galileo advocates, but on earlier incorrect speculations. Nevertheless, the Committee for the Nobel Prize in Physics was also misled as shown in their 1993 press release. Here, his errors are identified as related to accumulated mistakes in the field, and are illustrated with examples understandable at the undergraduate level. Another main problem is that many theorists failed to understand the principle of causality adequately. It is unprecedented to award a prize for mathematical errors. Keywords : Nobel Prize; general relativity; Einstein equation, Riemannian Space; the non- existence of dynamic solution; Galileo. GJSFR-A Classification : 04.20.-q, 04.20.Cv Comments on the 2011 Shaw Prize in Mathematical Sciences -- An Analysis of Collectively Formed Errors in Physics Strictly as per the compliance and regulations of : © 2012. -
Booklet 2008-09.Indd
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have achieved distinguished and significant advances, who have made outstanding contributions in culture and the arts, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference will be given to individuals whose significant work was recently achieved. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, is a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. In the 1950s he founded the film company Shaw Brothers (Hong Kong) Limited in Hong Kong. He has been Executive Chairman of Television Broadcasts Limited in Hong Kong since the 1970s. Mr Shaw has also founded two charities, The Sir Run Run Shaw Charitable Trust and The Shaw Foundation Hong Kong, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I am delighted to congratulate the six distinguished scientists who receive this year’s Shaw Prize. Their accomplishments enrich human knowledge and have a profound impact on the advancement of science. This year, the Shaw Prize recognises remarkable achievements in the areas of astronomy, life science and medicine, and mathematical sciences. The exemplary work and dedication of this year’s recipients vividly demonstrate that constant drive for excellence will eventually bear fruit. -
Professor Peter Goldreich Member of the Board of Adjudicators Chairman of the Selection Committee for the Prize in Astronomy
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have recently achieved distinguished and significant advances, who have made outstanding contributions in academic and scientific research or applications, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference is to be given to individuals whose significant work was recently achieved and who are currently active in their respective fields. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, was a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. During the 1950s he founded the film company Shaw Brothers (HK) Limited in Hong Kong. He was one of the founding members of Television Broadcasts Limited launched in Hong Kong in 1967. Mr Shaw also founded two charities, The Shaw Foundation Hong Kong and The Sir Run Run Shaw Charitable Trust, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I warmly congratulate the six Shaw Laureates of 2014. Established in 2002 under the auspices of Mr Run Run Shaw, the Shaw Prize is a highly prestigious recognition of the role that scientists play in shaping the development of a modern world. Since the first award in 2004, 54 leading international scientists have been honoured for their ground-breaking discoveries which have expanded the frontiers of human knowledge and made significant contributions to humankind. -
Science & ROGER PENROSE
Science & ROGER PENROSE Live Webinar - hosted by the Center for Consciousness Studies August 3 – 6, 2021 9:00 am – 12:30 pm (MST-Arizona) each day 4 Online Live Sessions DAY 1 Tuesday August 3, 2021 9:00 am to 12:30 pm MST-Arizona Overview / Black Holes SIR ROGER PENROSE (Nobel Laureate) Oxford University, UK Tuesday August 3, 2021 9:00 am – 10:30 am MST-Arizona Roger Penrose was born, August 8, 1931 in Colchester Essex UK. He earned a 1st class mathematics degree at University College London; a PhD at Cambridge UK, and became assistant lecturer, Bedford College London, Research Fellow St John’s College, Cambridge (now Honorary Fellow), a post-doc at King’s College London, NATO Fellow at Princeton, Syracuse, and Cornell Universities, USA. He also served a 1-year appointment at University of Texas, became a Reader then full Professor at Birkbeck College, London, and Rouse Ball Professor of Mathematics, Oxford University (during which he served several 1/2-year periods as Mathematics Professor at Rice University, Houston, Texas). He is now Emeritus Rouse Ball Professor, Fellow, Wadham College, Oxford (now Emeritus Fellow). He has received many awards and honorary degrees, including knighthood, Fellow of the Royal Society and of the US National Academy of Sciences, the De Morgan Medal of London Mathematical Society, the Copley Medal of the Royal Society, the Wolf Prize in mathematics (shared with Stephen Hawking), the Pomeranchuk Prize (Moscow), and one half of the 2020 Nobel Prize in Physics, the other half shared by Reinhard Genzel and Andrea Ghez. -
The Galactic Center: a Laboratory for Fundamental Astrophysics And
The Galactic Center: A Laboratory for Fundamental Astrophysics and Galactic Nuclei An Astro2010 Science White Paper Authors: Andrea Ghez (UCLA; [email protected]), Mark Morris (UCLA), Jessica Lu (Caltech), Nevin Weinberg (UCB), Keith Matthews (Caltech), Tal Alexander (Weizmann Inst.), Phil Armitage (U. of Colorado), Eric Becklin (Ames/UCLA), Warren Brown (CfA), Randy Campbell (Keck) Tuan Do (UCLA), Andrea Eckart (U. of Cologne), Reinhard Genzel (MPE/UCB), Andy Gould (Ohio State), Brad Hansen (UCLA), Luis Ho (Carnegie), Fred Lo (NRAO), Avi Loeb (Harvard), Fulvio Melia (U. of Arizona), David Merritt (RIT), Milos Milosavljevic (U. of Texas), Hagai Perets (Weizmann Inst.), Fred Rasio (Northwestern), Mark Reid (CfA), Samir Salim (NOAO), Rainer Sch¨odel (IAA), Sylvana Yelda (UCLA) Submitted to Science Frontier Panels on (1) The Galactic Neighborhood (GAN) arXiv:0903.0383v1 [astro-ph.GA] 2 Mar 2009 (2) Cosmology and Fundamental Physics (CFP) Supplemental Animations: http://www.astro.ucla.edu/∼ghezgroup/gc/pictures/Future GCorbits.shtml Galactic Center Stellar Dynamics Astro2010 White Paper 1 Abstract As the closest example of a galactic nucleus, the Galactic center presents an exquisite lab- oratory for learning about supermassive black holes (SMBH) and their environs. In this document, we describe how detailed studies of stellar dynamics deep in the potential well of a galaxy offer several exciting directions in the coming decade. First, it will be possible to obtain precision measurements of the Galaxy’s central potential, providing both a unique test of General Relativity (GR) and a detection of the extended dark matter distribution that is predicted to exist around the SMBH. Tests of gravity have not previously been pos- sible on scales larger than our solar system, or in regimes where the gravitational energy of a body is >∼1% of its rest mass energy. -
Works of Love
reader.ad section 9/21/05 12:38 PM Page 2 AMAZING LIGHT: Visions for Discovery AN INTERNATIONAL SYMPOSIUM IN HONOR OF THE 90TH BIRTHDAY YEAR OF CHARLES TOWNES October 6-8, 2005 — University of California, Berkeley Amazing Light Symposium and Gala Celebration c/o Metanexus Institute 3624 Market Street, Suite 301, Philadelphia, PA 19104 215.789.2200, [email protected] www.foundationalquestions.net/townes Saturday, October 8, 2005 We explore. What path to explore is important, as well as what we notice along the path. And there are always unturned stones along even well-trod paths. Discovery awaits those who spot and take the trouble to turn the stones. -- Charles H. Townes Table of Contents Table of Contents.............................................................................................................. 3 Welcome Letter................................................................................................................. 5 Conference Supporters and Organizers ............................................................................ 7 Sponsors.......................................................................................................................... 13 Program Agenda ............................................................................................................. 29 Amazing Light Young Scholars Competition................................................................. 37 Amazing Light Laser Challenge Website Competition.................................................. 41 Foundational -
Reversed out (White) Reversed
Berkeley rev.( white) Berkeley rev.( FALL 2014 reversed out (white) reversed IN THIS ISSUE Berkeley’s Space Sciences Laboratory Tabletop Physics Bringing More Women into Physics ALUMNI NEWS AND MORE! Cover: The MAVEN satellite mission uses instrumentation developed at UC Berkeley's Space Sciences Laboratory to explore the physics behind the loss of the Martian atmosphere. It’s a continuation of Berkeley astrophysicist Robert Lin’s pioneering work in solar physics. See p 7. photo credit: Lockheed Martin Physics at Berkeley 2014 Published annually by the Department of Physics Steven Boggs: Chair Anil More: Director of Administration Maria Hjelm: Director of Development, College of Letters and Science Devi Mathieu: Editor, Principal Writer Meg Coughlin: Design Additional assistance provided by Sarah Wittmer, Sylvie Mehner and Susan Houghton Department of Physics 366 LeConte Hall #7300 University of California, Berkeley Berkeley, CA 94720-7300 Copyright 2014 by The Regents of the University of California FEATURES 4 12 18 Berkeley’s Space Tabletop Physics Bringing More Women Sciences Laboratory BERKELEY THEORISTS INVENT into Physics NEW WAYS TO SEARCH FOR GOING ON SIX DECADES UC BERKELEY HOSTS THE 2014 NEW PHYSICS OF EDUCATION AND SPACE WEST COAST CONFERENCE EXPLORATION Berkeley theoretical physicists Ashvin FOR UNDERGRADUATE WOMEN Vishwanath and Surjeet Rajendran IN PHYSICS Since the Space Lab’s inception are developing new, small-scale in 1959, Berkeley physicists have Women physics students from low-energy approaches to questions played important roles in many California, Oregon, Washington, usually associated with large-scale of the nation’s space-based scientific Alaska, and Hawaii gathered on high-energy particle experiments. -
CV Bruce Beutler
Curriculum Vitae Prof. Dr. Bruce Beutler Name: Bruce Alan Beutler Born: 29 December 1957 Research focuses: Immune system, innate immunity, receptor proteins, toll gene, toll‐like receptors (TLR), tumour necrosis factor (TNF), TNF blockers Bruce Alan Beutler is an American immunologist and geneticist. In 2011 he was awarded the Nobel Prize in Physiology or Medicine along with Jules Hoffmann and Ralph M. Steinmann. The three scientists researched the human immune system and, as the Nobel committee put it, “revolutionised our understanding of the immune system”. Bruce Beutler and his colleague Jules Hoffmann discovered activation mechanisms of innate immunity. Academic and Professional Career since 2011 Director of the Center for the Genetics of Host Defense and holder of the “Raymond and Ellen Willie Distinguished Chair in Cancer Research”, University of Texas Southwestern Medical Center, USA 2007 ‐ 2011 Chief of the Department of Genetics, The Scripps Research Institute, La Jolla, USA 2000 ‐ 2007 Professor of Immunology and Microbial Science (IMS), The Scripps Research Institute, La Jolla, USA 2000 ‐ 2011 Lecturer, Kellogg School of Science and Technology, The Scripps Research Institute, La Jolla, USA 1996 ‐ 2000 Professor at the University of Texas Southwestern Medical Center, USA 1991 ‐ 2000 Associate Scientist at the University of Texas Southwestern Medical Center, USA 1990 ‐ 1996 Associate Professor, Department of Internal Medicine, University of Texas Southwestern Medical Center, USA Nationale Akademie der Wissenschaften Leopoldina www.leopoldina.org 1 1986 ‐ 1991 Assistant Investigator, Howard Hughes Medical Institute, USA 1986 ‐ 1990 Assistant Professor, Department of Internal Medicine, The University of Texas Southwestern Medical Center, USA 1985 ‐ 1986 Assistant Professor, Rockefeller University, USA 1983 ‐ 1985 Postdoctoral Fellow, Rockefeller University, USA 1981 ‐ 1983 Assistant, University of Texas Southwestern Medical Center, USA 1981 M.D., Pritzker School of Medicine, University of Chicago, USA 1976 B.A. -
Agenda Shaw-Workshop UTC
http://astro4edu.org/shaw-iau-workshops Tuesday 6th October 2020 UTC 14:00 – 15:30 Opening Event Markus Pössel IAU Office of Astronomy for Education, Germany Ewine van Dishoeck President of the International Astronomical Union (IAU), Leiden University, The Netherlands Theresia Bauer, MdL Chair of the Carl Zeiss Foundation Administration, Minister for Science, Research and Art of the State of Baden-Württemberg, Germany Beate Spiegel Managing Director of the Klaus Tschira Foundation, Germany Kenneth Young Chairman of the Shaw Prize Council and Vice Chair of the Board of Adjudicators, Shaw Prize Foundation, Hong Kong Teresa Lago General Secretary of the IAU, Portugal Keynote "Astronomy and Space Science: On top of Children’s interest" Svein Sjøberg, Professor in Science Education, Department of Teacher Education and School Research, University of Oslo, Norway Wednesday 7th October 2020 UTC 07:00 – 19:40 Session 4: Astronomy education resources (1h 40mins) UTC 07:00 – 08:40 UTC 07:00 – 07:10 Session Moderator Carolin Liefke, IAU Office of Astronomy for Education, Germany UTC 07:10 – 07:25 "Big Ideas in Astronomy" Pedro Russo, Leiden Observatory and Dep. Science Communication & Society, Leiden University, The Netherlands João Retrê, Institute of Astrophysics and Space Science, Portugal UTC 07:25 – 07:40 "astroEDU: an astronomy activity repository. Developments over 2020" Michael Fitzgerald, Edith Cowan University Perth, Australia UTC 07:40 – 07:55 "Considerations on the importance of building a national astronomical glossary: the Japanese -
On the Hunt for Excited States
INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 45 NUMBER 10 DECEMBER 2005 On the hunt for excited states HOMESTAKE DARK MATTER SNOWMASS Future assured for Galactic gamma rays US workshop gets underground lab p5 may hold the key p 17 ready for the ILC p24 www.vectorfields.comi Music to your ears 2D & 3D electromagnetic modellinj If you're aiming for design excellence, demanding models. As a result millions you'll be pleased to hear that OPERA, of elements can be solved in minutes, the industry standard for electromagnetic leaving you to focus on creating modelling, gives you the most powerful outstanding designs. Electron trajectories through a TEM tools for engineering and scientific focussing stack analysis. Fast, accurate model analysis • Actuators and sensors - including Designed for parameterisation and position and NDT customisation, OPERA is incredibly easy • Magnets - ppm accuracy using TOSCA to use and has an extensive toolset, making • Electron devices - space charge analysis it ideal for a wide range of applications. including emission models What's more, its high performance analysis • RF Cavities - eigen modes and single modules work at exceptional levels of speed, frequency response accuracy and stability, even with the most • Motors - dynamic analysis including motion Don't take our word for it - order your free trial and check out OPERA yourself. B-field in a PMDC motor Vector Fields Ltd Culham Science Centre, Abingdon, Oxon, 0X14 3ED, U.K. Tel: +44 (0)1865 370151 Fax: +44 (0)1865 370277 Email: [email protected] Vector Fields Inc 1700 North Famsworth Avenue, Aurora, IL, 60505. -
Honors and Awards Recipients, One of My Favorite Commencement Traditions Is Recognizing the Academic Excellence of Our Students During the Honors and Awards Program
onors and wards H 2021A HonorsINTRODUCTION and Awards Dr. Michele Gillespie, Dean, Wake Forest College To our 2021 College Honors and Awards recipients, One of my favorite Commencement traditions is recognizing the academic excellence of our students during the Honors and Awards program. While we are unable to celebrate together in-person this year, I want to congratulate our students for their impressive achievements in the arts, humanities, social sciences, and sciences through this commemorative program. The honors and awards listed here represent thousands of hours of research, scholarship, and critical thinking. These students have demonstrated intellectual leadership, contributed to the creation of new knowledge, expressed themselves creatively through different mediums, and produced strikingly original scholarship. Class of 2021, you have fulfilled the mission that we set before you when you first stood in Wait Chapel during opening convocation four years ago. We told you then to use your liberal arts education to build a pro humanitate spirit that will let you make the world a better place for all. Your intellectual curiosity, passion for knowledge, and concern for others inspires all around you, including your parents, your faculty, and me. Thank you to our faculty for carefully guiding these students along the path to academic excellence. Parents and families, I salute your efforts as well. You have been beacons of love and support. I know we are all proud of these students because they know how to ask critical questions. “The power to question,” Indira Gandhi observed, “is the basis of all human progress.” May you continue to question our world, and to use knowledge to change what you do not like in our world so you can make it better. -
The Observatory Founded in 1877 by Sir William Christie, Astronomer Royal
The Observatory Founded in 1877 by Sir William Christie, Astronomer Royal EditEd by D. J. SticklanD R. W. ARgyle S. J. Fossey eDitors 1877–2013 W. H. m. Christie 1877–1882 P. J. d. Gething 1954–1956 E. W. maunder 1881–1887 d. W. dewhirst 1956–1957 A. m. W. downing 1885–1887 A. Hewish 1957–1961 t. lewis 1885–1887 W. R. Hindmarsh 1957–1961 and 1893–1912 b. E. J. Pagel 1961–1962 A. A. Common 1888–1892 J. E. baldwin 1961–1962 H. H. turner 1888–1897 d. mcNally 1961–1963 H. P. Hollis 1893–1912 C. A. murray 1961–1966 S. Chapman 1913–1914 P. A. Wayman 1962–1964 A. S. Eddington 1913–1919 R. V. Willstrop 1963–1966 F. J. m. Stratton 1913–1925 R. F. Griffin 1963–1985 H. Spencer Jones 1915–1923 J. b. Alexander 1964–1965 J. Jackson 1920–1927 S. V. m. Clube 1965–1966 W. m. H. Greaves 1924–1932 K. b. Gebbie 1966–1968 J. A. Carroll 1926–1931 W. Nicholson 1966–1973 G. merton 1928 d. lynden-bell 1967–1969 W. H. Steavenson 1929–1933 C. Jordan 1968–1973 H. W. Newton 1929–1936 R. G. bingham 1969–1972 R. o. Redman 1932–1935 m. V. Penston 1972–1975 R. v. d. R. Woolley 1933–1939 S. J. burnell 1973–1976 W. H. mcCrea 1935–1937 d. H. P. Jones 1973–1977 H. F. Finch 1936–1947 P. J. Andrews 1975–1983 A. d. thackeray 1938–1942 G. G. Pooley 1976–1984 G. C. mcVittie 1938–1948 R.