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2015 Annual Report
2015 AMERICAN PHYSICAL SOCIETY ANNUAL TM ADVANCING PHYSICS REPORT TM THE AMERICAN PHYSICAL SOCIETY STRIVES TO Be the leading voice for physics and an authoritative source of physics information for the advancement of physics and the benefit of humanity Collaborate with national scientific societies for the advancement of science, science education, and the science community Cooperate with international physics societies to promote physics, to support physicists worldwide, and to foster international collaboration Have an active, engaged, and diverse membership, and support the activities of its units and members © 2016 American Physical Society During 2015, APS worked to institute the governance objective: “the advancement and diffusion of the knowledge changes approved by the membership in late 2014. In of physics.” APS is fully committed to the principles of OA accordance with the new Constitution & Bylaws, in to the extent that we can continue to support the production February the Board appointed our first Chief Executive of high-quality peer-reviewed journals. For many years APS Officer—Kate Kirby, the former Executive Officer—to has supported “green” OA and we have been fully compliant head the APS. Kate’s major task has been to transition with the 2013 directive from the Office of Science and the management of APS to a CEO model with a Senior Technology Policy that the publications resulting from Management Team. She appointed Mark Doyle as Chief U.S. federally funded research be accessible to the public 12 Information Officer, James Taylor as Chief Operating months after publication. Since APS is a major international Officer, and Matthew Salter as the new Publisher. -
HOPE Meetings Are Held for Excellent Graduate Students and Young Researchers Specially Selected from Countries Around the 9Th Asia-Pacific and Africa Region
For Overseas Cooperating Institutions Objective HOPE Meetings are held for excellent graduate students and young researchers specially selected from countries around the 9th Asia-Pacific and Africa region. These meetings give an opportunity for the participants to engage in interdisciplinary discussions with Nobel laureates and other distinguished HOPE MEETING scientists pioneering the frontiers of knowledge. They also give the participants, who lodge together over the course of the event, a chance to make friends and form collegial networks with Nobel Laureates with peers from the regions. The title “HOPE Meeting” signifies the promise held for the future roles of young researchers and optimism for creating a bright S&T future within the global community. Date F ebruary 26- ■ Saturday, February 25: Orientation & Registration M arch 2, 2017 ■ Sunday, February 26: Nobel Prize Dialogue Tokyo 2017 Organizer Venue Tokyo , JAPAN Office of the HOPE Meetings, JSPS E-mail [email protected] Tel: +81-3-3263-2414 Fax:+81-3-3234-3700 HOPE MEETINGS with Nobel Laureates Organizing Committee of the HOPE Meetings ■ Chair Makoto Kobayashi <Nobel Laureate in Physics 2008> Honorary Professor Emeritus, High Energy Accelerator Research Organization (KEK) ■ Members Noriko Osumi Mitsuhiko Shionoya Tohoku University The University of Tokyo Takaaki Kajita <Nobel Laureate in Physics 2015> Yousuke Takahama The University of Tokyo Tokushima University Kazuhiro Kosuge Fumio Hanaoka Tohoku University Tsukuba University Program of the HOPE Meeting The program -
Panel Discussion on the Nobel Prize in Physics 2015 Tommy Ohlsson Motivation for the Nobel Prize in Physics 2015
KTH ROYAL INSTITUTE OF TECHNOLOGY Panel Discussion on the Nobel Prize in Physics 2015 Tommy Ohlsson Motivation for the Nobel Prize in Physics 2015 The Nobel Prize in Physics 2015 was awarded jointly to Takaaki Kajita and Arthur B. McDonald "for the discovery of neutrino oscillations, which shows that neutrinos have mass" Takaaki Kajita Arthur B. McDonald (Super-Kamiokande) (SNO) Motivation for the Nobel Prize in Physics 2015 The Nobel Prize in Physics 2015 was awarded jointly to Takaaki Kajita and Arthur B. McDonald "for the discovery of neutrino oscillations, which shows that neutrinos have mass" Ed Kearns Takaaki Kajita Arthur B. McDonald Dave Wark (Super-Kamiokande) (Super-Kamiokande) (SNO) (SNO) Super-Kamiokande (in Japan) In June 1998, the Super-Kamiokande collaboration presented its first results of measurements of atmospheric neutrinos that give evidence for neutrino oscillations (i.e. quantum mechanical effects over distances of thousands of kilometers). This result is the first solid evidence for physics beyond the Standard Model of particle physics. The atmospheric neutrino analysis of the Super-Kamiokande collaboration was led by Takaaki Kajita. SNO (in Canada) In April 2002, the SNO collaboration presented the first direct measurement of the total flux of all active boron-8 neutrinos arriving from the Sun, which provided additional evidence for neutrino flavor transitions. The SNO collaboration was led by Art McDonald. ) -1 8 SNO SNO s q q -2 7 ES CC cm 6 6 (10 o 5 µ q SNO 4 qNC 3 qSSM 2 1 0 0123456 6 -2 -1 qe (10 cm s ) Other neutrino oscillation experiments • KamLAND • first results on anti-electron neutrino flux from distant nuclear reactors • demonstrated disappearance of anti-electron neutrinos and showed that the LMA solution is the only remaining solar neu. -
Communications-Mathematics and Applied Mathematics/Download/8110
A Mathematician's Journey to the Edge of the Universe "The only true wisdom is in knowing you know nothing." ― Socrates Manjunath.R #16/1, 8th Main Road, Shivanagar, Rajajinagar, Bangalore560010, Karnataka, India *Corresponding Author Email: [email protected] *Website: http://www.myw3schools.com/ A Mathematician's Journey to the Edge of the Universe What’s the Ultimate Question? Since the dawn of the history of science from Copernicus (who took the details of Ptolemy, and found a way to look at the same construction from a slightly different perspective and discover that the Earth is not the center of the universe) and Galileo to the present, we (a hoard of talking monkeys who's consciousness is from a collection of connected neurons − hammering away on typewriters and by pure chance eventually ranging the values for the (fundamental) numbers that would allow the development of any form of intelligent life) have gazed at the stars and attempted to chart the heavens and still discovering the fundamental laws of nature often get asked: What is Dark Matter? ... What is Dark Energy? ... What Came Before the Big Bang? ... What's Inside a Black Hole? ... Will the universe continue expanding? Will it just stop or even begin to contract? Are We Alone? Beginning at Stonehenge and ending with the current crisis in String Theory, the story of this eternal question to uncover the mysteries of the universe describes a narrative that includes some of the greatest discoveries of all time and leading personalities, including Aristotle, Johannes Kepler, and Isaac Newton, and the rise to the modern era of Einstein, Eddington, and Hawking. -
Nobel Prize 2015 , Vol
The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics 2015 to Takaaki Kajita and Arthur B. McDonald “for the discovery of neutrino oscillations, which shows that The Nobel Prize 2015 in Physics neutrinos have mass”. the Nobel Foundation. Nobel the Nobel Prize® and the Nobel Prize® medal design mark are registered trademarks of Only electron neutrinos Atmospheric neutrinos are produced in the Sun. are produced in collisions between Chameleons cosmic rays and the Earth’s atmosphere. of space Takaaki Kajita in Japan and Arthur B. McDonald in Canada were key scientists in two large research groups that discovered that neutrinos change identities, which requires that neutrinos have mass. The discovery has changed our understanding of the innermost workings of matter and may prove crucial to our view of the universe. B The discovery of neutrino identity changes between cosmic radiation and the Earth's A Sudbury Neutrino Observatory has resolved a neutrino puzzle that physicists atmosphere. Others are produced in nuclear The detector measured neutrinos from the Sun. had wrestled with for decades. Compared reactions inside the Sun. Thousands of billions Its tank, filled with heavy water, was placed to theoretical calculations of the number of neutrinos stream through our bodies every two kilometres under the surface of the Earth. of neutrinos, up to two-thirds of them were second. The combined weight of neutrinos Signals from all three types of neutrinos were missing in measurements performed on Earth. is estimated to be roughly equal to that of all registered in the tank. The sum of the neutrinos The two research groups discovered that the visible stars in the universe. -
Research in Kamioka and Kakenhi Takaaki Kajita Director of Institute for Cosmic Ray Research (ICRR) the University of Tokyo Rese
Research in Kamioka and Kakenhi Takaaki Kajita Director of Institute for Cosmic Ray Research (ICRR) The University of Tokyo Research Theme Implemented in FY2017: First Detection of Gravitational Waves Using Cryogenic Laser Interferometer (Grant-in-Aid for Specially Promoted Research) I have conducted research underground Kamioka, Gifu Prefecture, since I was a graduate student. The first experiment I participated in was the Kamioka Nucleon Decay Experiment (Kamiokande). The experiment was initially proposed by Professor Masatoshi Koshiba, who was my thesis advisor, to search for proton decay. Professor Koshiba collaborated with a company to develop an unprecedentedly large 50-centimeter diameter photomultiplier tube (PMT) for the Kamiokande experiment. The PMT served a very important role in supernova neutrino observations that verified the supernova explosion mechanism and solar neutrino observations that confirmed the so-called solar neutrino problem. It is well known that, due to these achievements, Professor Koshiba received the Nobel Prize in physics in 2002. It is common for a large apparatus such as this to be realized by submitting a budget request from a host institute after long, vigorous discussions in relevant researcher communities. In this case, however, the enthusiasm of the relevant researchers in view of the importance of Kamiokande experiments made it possible to realize the experiment quickly with funds from various sources. Kamiokande initially materialized through collaboration with the University of Tokyo’s School of Science, to which Professor Koshiba belonged, the former National Laboratory for High Energy Physics (KEK), and the Institute for Cosmic Ray Research (ICRR) of the University of Tokyo. Although I was only a graduate student at that time and knew nothing about budgets, all of us participating in the effort recognized that people thought that this experiment was very important and endeavored to realize it as soon as possible. -
The Future of Fermilab
CERN & Fermilab LHC & Neutrinos Nigel S. Lockyer CERN Council 3/16/2015 P5 Report…still very impactful in Washington • P5 report has had and is having a major impact on US planning for particle physics because: – Excellent report that made difficult choices and has focused field – Community support very high • Secretary of Energy has expressed strong support for report because of community support • P5 top priorities: LHC and Neutrinos Nigel Lockyer | CERN Council 2015 CERN/DOE Agreement: The Signers…Moniz, Heuer, Cordova Nigel Lockyer | CERN Council 2015 CERN & Fermilab….together we are stronger • CERN is the world’s leading high energy lab now that Fermilab has relinquished the energy frontier with closing of Tevatron • CERN is mandated to “steward” all European particle physics • Fermilab is only “single program” HEP laboratory in US • CERN needs the US to execute the HL-LHC successfully and we need CERN to help with LBNF • By supporting a world class long baseline neutrino program in US, CERN is supporting the European neutrino community • CERN and Fermilab both have tremendous technical depth • Interests & technology overlap on FCC • Success of both CERN & Fermilab are highly intertwined Nigel Lockyer | CERN Council 2015 NY Times:U.S. & European Scientists Sign Cooperation Pact • “a model for the kinds of international scientific collaboration that can enable breakthrough insights and innovations.”…John Holdren, President’s Science Advisor • “This agreement is also historic since it formalizes CERN’s participation in U.S.-based programs such as prospective future neutrino facilities for the first time.” Rolf Heuer DG CERN • “Our research programs in the U.S. -
Report and Opinion 2016;8(6) 1
Report and Opinion 2016;8(6) http://www.sciencepub.net/report Beyond Einstein and Newton: A Scientific Odyssey Through Creation, Higher Dimensions, And The Cosmos Manjunath R Independent Researcher #16/1, 8 Th Main Road, Shivanagar, Rajajinagar, Bangalore: 560010, Karnataka, India [email protected], [email protected] “There is nothing new to be discovered in physics now. All that remains is more and more precise measurement.” : Lord Kelvin Abstract: General public regards science as a beautiful truth. But it is absolutely-absolutely false. Science has fatal limitations. The whole the scientific community is ignorant about it. It is strange that scientists are not raising the issues. Science means truth, and scientists are proponents of the truth. But they are teaching incorrect ideas to children (upcoming scientists) in schools /colleges etc. One who will raise the issue will face unprecedented initial criticism. Anyone can read the book and find out the truth. It is open to everyone. [Manjunath R. Beyond Einstein and Newton: A Scientific Odyssey Through Creation, Higher Dimensions, And The Cosmos. Rep Opinion 2016;8(6):1-81]. ISSN 1553-9873 (print); ISSN 2375-7205 (online). http://www.sciencepub.net/report. 1. doi:10.7537/marsroj08061601. Keywords: Science; Cosmos; Equations; Dimensions; Creation; Big Bang. “But the creative principle resides in Subaltern notable – built on the work of the great mathematics. In a certain sense, therefore, I hold it astronomers Galileo Galilei, Nicolaus Copernicus true that pure thought can -
Highlights of Modern Physics and Astrophysics
Highlights of Modern Physics and Astrophysics How to find the “Top Ten” in Physics & Astrophysics? - List of Nobel Laureates in Physics - Other prizes? Templeton prize, … - Top Citation Rankings of Publication Search Engines - Science News … - ... Nobel Laureates in Physics Year Names Achievement 2020 Sir Roger Penrose "for the discovery that black hole formation is a robust prediction of the general theory of relativity" Reinhard Genzel, Andrea Ghez "for the discovery of a supermassive compact object at the centre of our galaxy" 2019 James Peebles "for theoretical discoveries in physical cosmology" Michel Mayor, Didier Queloz "for the discovery of an exoplanet orbiting a solar-type star" 2018 Arthur Ashkin "for groundbreaking inventions in the field of laser physics", in particular "for the optical tweezers and their application to Gerard Mourou, Donna Strickland biological systems" "for groundbreaking inventions in the field of laser physics", in particular "for their method of generating high-intensity, ultra-short optical pulses" Nobel Laureates in Physics Year Names Achievement 2017 Rainer Weiss "for decisive contributions to the LIGO detector and the Kip Thorne, Barry Barish observation of gravitational waves" 2016 David J. Thouless, "for theoretical discoveries of topological phase transitions F. Duncan M. Haldane, and topological phases of matter" John M. Kosterlitz 2015 Takaaki Kajita, "for the discovery of neutrino oscillations, which shows that Arthur B. MsDonald neutrinos have mass" 2014 Isamu Akasaki, "for the invention of -
Professor Takaaki Kajita Donates Two Types of Photomultiplier Tubes to the Nobel Museum
Professor Takaaki Kajita donates two types of photomultiplier tubes to the Nobel Museum December 6, 2015 — 2015 Nobel Laureate Professor Takaaki Kajita, Director of the University of Tokyo Institute for Cosmic Ray Research, has donated two types of photomultiplier tubes to the Nobel Museum in Stockholm as artifacts related to his research. A photomultiplier tube is a type of photosensor used in the Super-Kamiokande experiment at the Kamioka Observatory in central Japan. Professor Kajita has donated one sensor each from the Super-Kamiokande inner and outer detectors to the museum. The Super-Kamiokande detector is filled with 50,000 tons of purified water and is divided into an inner detector, which holds 32,000 tons, and a two meter-wide outer detector that contains the remainder (Figure 1). The wall of the inner detector is lined with around 11,000 photomultiplier tubes, each with a 20 inch (50 cm) diameter (Figure 2), that detect Cherenkov light originating from reactions between neutrinos and water in the inner detector. The 20-inch photomultiplier tube was first developed in 1981 by Hamamatsu Photonics K.K. in collaboration with the University of Tokyo and KEK for the Kamiokande detector. The photomultiplier tubes used in the Super-Kamiokande detector are the result of continuous improvements to this original model. In 2014 the 20-inch photomultiplier tube was recognized with an IEEE milestone award. IEEE Milestones in Electrical Engineering and Computing honor significant technical achievements in electrical, electronics, informatics and communications fields. The outer detector is fitted with 1,885 photomultiplier tubes that are 8 inches (20 cm) in diameter (Figure 3). -
Tevatron Physics
Tevatron Physics Welcome new Fermilab director Nigel Lockyer Reinhard Schwienhorst Outline • Tevatron proton-antiproton collider • Heavy flavor production • QCD events • Electroweak results • Top quark measurements • Higgs boson coupling to fermions • Conclusions 2 Reinhard Schwienhorst Tevatron at Fermilab •Run II from 2002 to 2011 •CDF and D0: 400 + 400 members from 60 + 70 institutions 3 Reinhard Schwienhorst Tevatron collider in Run II • proton-antiproton collider • 1.96 TeV • 12 fb-1 delivered • 10 fb-1 recorded per experiment • 10 pByte dataset (incl. MC) per experiment 4 Reinhard Schwienhorst Unique Tevatron physics • proton-antiproton collider - quark-antiquark interactions - top pairs - forward-backward asymmetries - single top in the s-channel • lower CM energy - Higgs to bb in associated production - lower QCD background - coupling to fermions • Much less pileup than LHC - clean events, low trigger thresholds - precision top quark mass - precision W boson mass 5 Reinhard Schwienhorst Heavy flavor physics • Trigger and detector systems for heavy flavor - low-pT di-muons and regular reversal of B field (DØ) - track trigger and high-precision tracking (CDF) 6 Reinhard Schwienhorst CP Asymmetries • Tevatron Proton-Antiproton initial state - CP conserving • Look for neutral meson mixing • Look for asymmetries in heavy flavor decay rates • Sensitive to new physics - in weak and strong interactions 7 Reinhard Schwienhorst Like-sign di-muon asymmetry • DØ di-muon asymmetry in semi-leptonic B decays - Significance 3.9 s.d. PRD 84, 052007 -
Neutrinos Are Everywhere: Towards a New Understanding of the Quantum Universe
Neutrinos are Everywhere: Towards a New Understanding of the Quantum Universe Nigel S. Lockyer Princeton University 6/17/2016 2 Nigel Lockyer | Princeton June 2016 First Baby Bison Arrives 2016…National Mammal… 3 Nigel Lockyer | Princeton June 2016 Government wants to check they are Bison Recent Genetic Analysis of Herd…they are bison 4 Nigel Lockyer | Princeton June 2016 Coyotes down selected in national mammal competition 5 Nigel Lockyer | Princeton June 2016 International Particle Physics Community Convergence • 2013: European Strategy for Particle Physics updated - Endorsed high priority of neutrino physics - Bottom line: CERN should help the European neutrino community participate in a long-baseline program outside of Europe • 2014: “P5” Plan - A strategic plan for U.S. particle physics maximizing opportunities for breakthrough science - Explicit prioritization, hard choices made within realistic budget scenarios - Particle physics community unified behind the plan: 2,331 signatures on letter sent to Secretary Moniz 6 Nigel Lockyer | Princeton June 2016 CERN/DOE/NSF Agreement: Signers…Moniz, Heuer, Cordova 7 Nigel Lockyer | Princeton June 2016 Neutrino Protocol…signed recently at CERN CERN and Fermilab’s futures are completely intertwined for next several decades …..as never before 8 Nigel Lockyer | Princeton June 2016 Major news: Signing of US-CERN Protocols In December, the United States and the European physics laboratory CERN signed an agreement to partner on continued research at the Large Hadron Collider, upcoming neutrino research