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Research Article an Appraisal of Muon Neutrino Disappearance at Short Baseline
Hindawi Publishing Corporation Advances in High Energy Physics Volume 2013, Article ID 948626, 11 pages http://dx.doi.org/10.1155/2013/948626 Research Article An Appraisal of Muon Neutrino Disappearance at Short Baseline L. Stanco,1 S. Dusini,1 A. Longhin,2 A. Bertolin,1 and M. Laveder3 1 INFN-Padova, Via Marzolo 8, 35131 Padova, Italy 2 Laboratori Nazionali di Frascati, INFN, Via E. Fermi 40, 00044 Frascati, Italy 3 Padova University and INFN-Padova, Via Marzolo 8, 35131 Padova, Italy Correspondence should be addressed to L. Stanco; [email protected] Received 20 June 2013; Revised 12 September 2013; Accepted 6 October 2013 Academic Editor: Kate Scholberg Copyright © 2013 L. Stanco et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Neutrino physics is nowadays receiving more and more attention as a possible source of information for the long-standing problem of new physics beyond the Standard Model. The recent measurement of the third mixing angle 13 in the standard mixing oscillation scenario encourages us to pursue the still missing results on leptonic CP violation and absolute neutrino masses. However, several puzzling measurements exist which deserve an exhaustive evaluation. Wewill illustrate the present status of the muon disappearance measurements at small / and the current CERN project to revitalize the neutrino field in Europe with emphasis on the search for sterile neutrinos. We will then illustrate the achievements that a double muon spectrometer can make with regard to discovery of new neutrino states, using a newly developed analysis. -
Puzzling out Neutrino Mixing Through Golden Measurements
Universidad Aut´onoma de Madrid Facultad de Ciencias Departamento de F´ısica Te´orica Puzzling out neutrino mixing through golden measurements Memoria de Tesis Doctoral realizada por Olga Mena Requejo, presentada ante el Departamento de F´ısica Te´orica de la Universidad Aut´onoma de Madrid para la obtenci´on del T´ıtulo de Doctora en Ciencias. Tesis Doctoral dirigida por la Catedr´atica M. Bel´en Gavela Legazpi, del Departamento de F´ısica Te´orica de la Universidad Aut´onoma de Madrid Madrid, Noviembre 2002. Agradecimientos “Erase´ una vez....” siempre me ha fascinado el principio de los cuentos infantiles (era el ´unico susurro que lograba escuchar segundos antes de conciliar el sue˜no), pero hoy intentar´emantenerme despierta..., una taza de caf´e, un bostezo,..., y seguro que yo tambi´en puedo contar un buen cuento, como mis abuelas...voy a intentarlo... “....una estudiante de F´ısicas, una entre los (400) j´ovenes estudiantes que se ma- triculan cada a˜no en la Universidad Aut´onoma∼O de Madrid, UAM para los amigos. Durante su tercer y cuarto a˜no de estudios, curs´ociertas asignaturas que realmente le impactaron, como la Mec´anica Cu´antica y la Mec´anica Te´orica. Un a˜no antes de li- cenciarse, acudi´oal despacho de la que hab´ıasido su profesora de Mec´anica Cu´antica, Bel´en Gavela, y le pregunt´oacerca de seguir investigando en F´ısica Te´orica con su ayuda. Bel´en la apoy´oy anim´o, la escuch´oy discuti´ocon ella cada tema que estudi- aba, le cedi´olibros, art´ıculos y trat´ode desnudar la F´ısica ante sus ojos. -
A Summer with the Large Hadron Collider: the Search for Fundamental Physics
University of New Hampshire University of New Hampshire Scholars' Repository Inquiry Journal 2009 Inquiry Journal Spring 2009 A Summer with the Large Hadron Collider: The Search for Fundamental Physics Austin Purves University of New Hampshire Follow this and additional works at: https://scholars.unh.edu/inquiry_2009 Part of the Physics Commons Recommended Citation Purves, Austin, "A Summer with the Large Hadron Collider: The Search for Fundamental Physics" (2009). Inquiry Journal. 14. https://scholars.unh.edu/inquiry_2009/14 This Article is brought to you for free and open access by the Inquiry Journal at University of New Hampshire Scholars' Repository. It has been accepted for inclusion in Inquiry Journal 2009 by an authorized administrator of University of New Hampshire Scholars' Repository. For more information, please contact [email protected]. UNH UNDERGRADUATE RESEARCH JOURNAL SPRING 2009 research article A Summer with the Large Hadron Collider: the Search for Fundamental Physics —Austin Purves (Edited by Aniela Pietrasz and Matthew Kingston) For centuries people have pushed the boundaries of observational science on multiple fronts. Our ability to peer ever more deeply into the world around us has helped us to understand it: telescopes and accurate measurement of planetary motion helped us to break free from the earth–centered model of the solar system; increasingly powerful microscopes allowed us to see how our bodies work as a collection of tiny cells; particle colliders allowed us to better understand the structure of atoms and the interactions of subatomic particles. Construction of the latest and most powerful particle collider, the Large Hadron Collider (LHC), was completed in fall 2008 at Conseil Européen pour la Recherche Nucléaire (CERN), the world’s largest particle physics research center, located near Geneva, Switzerland. -
The PLUTO Experiment at DORIS (DESY) and the Discovery of the Gluon (A Recollection]
(9.46 GeV) and the gluon discovery (a critical recollection of PLUTO results)* Bruno R. Stella1,a and Hans-Jürgen Meyer2,b 1 Department of Physics of Roma Tre University and INFN; Rome, Italy 2 formerly at Department of Physics, Siegen University; Siegen, Germany Abstract. The hadronic decays of (9.46 GeV) were first studied by the PLUTO experiment at the DORIS e+e- storage ring (DESY). With the aim of determining the contribution of PLUTO to the discovery of the gluon, as members of this former collaboration we have reconsidered all the scientific material produced by PLUTO in 1978 and the first half of 1979. It results clearly that the experiment demonstrated the main decay of the (9.46 GeV) resonance to be mediated by 3 gluons, by providing evidence for the agreement of this hypothesis with average values and differential distributions of all possible experimental variables and by excluding all other possible alternative models. Jettiness resulted evident by the average transverse momentum <pT> with respect to the event thrust axis, which was the same as experimentally observed by PLUTO itself at nearby continuum c.m.s. energies for 2-quark jet events. On the contrary, the average sphericity <S> and more topological variables as well as the momentum distribution showed a net difference with the same data comparison, a result compatible with jettiness only in case of more than 2 jets. Flatness as consequence of a 3-body decay (therefore 3 jets) was indicated by the low average momentum out of the event plane <pout>, altogether a result being independent of models. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
Jet Production and High Pt Phenomena in Photon-Photon Reactions*
JET PRODUCTION AND HIGH PT PHENOMENA IN PHOTON-PHOTON REACTIONS* NORBERT WERMES ~" Stanford Linear Accelerator Center Stanford University, Stanford, California 94305 ABSTRACT The status of experimental investigations of high PT phenomena and jet production in photon- photon collisions is reviewed. Taking the challenging questions on hard scattering processes in ~/ff reactions as a guide, the experimental approach to these questions is summarized. Results from the PETRA experiments CELLO, JADE, PLUTO, and TASSO are presented including preliminary results on the Q2-dependence of jet cross sections. Experimental limitations and background problems are discussed. Zusammenfassung -- Es wird ein Uberblick fiber den Stand experimenteller Untersuchungen yon high-PT Ph~nomenen und der Erzeugung von Jets in Photon-Photon Wechselwirkungen gegeben. Anhand der herausfordernden Fragen beziiglich harter Streuprozesse in ~/ff Reaktionen wird der experimentelle Ansatz zur Beantwortung dieser Fragen zusammengefasst. Ergebnisse der PETRA Experimente CELLO, JADE, PLUTO und TASSO werden presentiert. Vorli~ufige Untersuchungen der Q2-Abh~ngigkeit von Jet-Wirkungsquerschnitten sowie experimentelle Einschr~nkungen und Untergrundprobleme werden diskutiert. * Work supported by the Department of Energy, contract DE-AC03-76SF00515. ? Alexander yon Humboldt Fellow. 120 1. INTRODUCTION This talk reviews experimental results on hard scattering reactions in qff collisions via high PT phenomena. The talk is divided into three parts. First I shall try to list the physics challenges for photon- photon experiments, in the context of hard scattering processes at high PT. In the main part the experimental approach to these challenging questions is discussed. It will be explained why we believe that hard scattering processes do exist. Then the explicit jet-searches performed by the different experiments are reviewed. -
New Physics with Neutrinos
New Physics with Neutrinos Dissertation zur Erlangung des Grades \Doktor der Naturwissenschaften" am Fachbereich Physik, Mathematik und Informatik der Johannes Gutenberg-Universitat¨ in Mainz Mona Inge Dentler geboren in Munchen¨ Mainz, den 23.11.2018 Abstract Due to open problems in theory and unresolved anomalies in various oscilla- tion experiments, neutrino physics appears to be an excellent starting point in the quest for physics beyond the Standard Model (SM). The 3 + 1 framework featuring an additional, sterile neutrino mixing with the known neutrinos, is a minimalist extension of the SM which can account for oscillation phenomenology beyond the standard three flavor paradigm. However, two orthogonal arguments militate against this model. First, the increasing amount of ambiguous experimental results makes a con- sistent interpretation of the data in the 3 + 1 framework appear unlikely. In this regard, global fits provide a useful tool to investigate this objection. This thesis reports on the results of an up-to-date global fit to all relevant, available datasets, including the data corresponding to the reactor antineutrino anomaly (RAA), the gallium anomaly and the short baseline (SBL) anomaly. The reactor data as a special case can plausibly be explained by the hypothesis of a misprediction of the reactor antineutrino flux. Therefore, this hypothesis is tested against the 3 + 1 framework. Both hypotheses are found to be similarly likely, with a slight preference for the 3 + 1 framework, mainly driven by the data from DANSS and NEOS, which measure antineutrino spectra. However, a combination of both hypotheses fits the data best, with the hypothesis of a mere misprediction of the reactor flux rejected at 2:9σ. -
MIT at the Large Hadron Collider—Illuminating the High-Energy Frontier
Mit at the large hadron collider—Illuminating the high-energy frontier 40 ) roland | klute mit physics annual 2010 gunther roland and Markus Klute ver the last few decades, teams of physicists and engineers O all over the globe have worked on the components for one of the most complex machines ever built: the Large Hadron Collider (LHC) at the CERN laboratory in Geneva, Switzerland. Collaborations of thousands of scientists have assembled the giant particle detectors used to examine collisions of protons and nuclei at energies never before achieved in a labo- ratory. After initial tests proved successful in late 2009, the LHC physics program was launched in March 2010. Now the race is on to fulfill the LHC’s paradoxical mission: to complete the Stan- dard Model of particle physics by detecting its last missing piece, the Higgs boson, and to discover the building blocks of a more complete theory of nature to finally replace the Standard Model. The MIT team working on the Compact Muon Solenoid (CMS) experiment at the LHC stands at the forefront of this new era of particle and nuclear physics. The High Energy Frontier Our current understanding of the fundamental interactions of nature is encap- sulated in the Standard Model of particle physics. In this theory, the multitude of subatomic particles is explained in terms of just two kinds of basic building blocks: quarks, which form protons and neutrons, and leptons, including the electron and its heavier cousins. From the three basic interactions described by the Standard Model—the strong, electroweak and gravitational forces—arise much of our understanding of the world around us, from the formation of matter in the early universe, to the energy production in the Sun, and the stability of atoms and mit physics annual 2010 roland | klute ( 41 figure 1 A photograph of the interior, central molecules. -
Asteroid Regolith Weathering: a Large-Scale Observational Investigation
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2019 Asteroid Regolith Weathering: A Large-Scale Observational Investigation Eric Michael MacLennan University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Recommended Citation MacLennan, Eric Michael, "Asteroid Regolith Weathering: A Large-Scale Observational Investigation. " PhD diss., University of Tennessee, 2019. https://trace.tennessee.edu/utk_graddiss/5467 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Eric Michael MacLennan entitled "Asteroid Regolith Weathering: A Large-Scale Observational Investigation." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Joshua P. Emery, Major Professor We have read this dissertation and recommend its acceptance: Jeffrey E. Moersch, Harry Y. McSween Jr., Liem T. Tran Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Asteroid Regolith Weathering: A Large-Scale Observational Investigation A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Eric Michael MacLennan May 2019 © by Eric Michael MacLennan, 2019 All Rights Reserved. -
The Long-Baseline Neutrino Facility: Building the Future
Fermi National Accelerator Laboratory July 2017 The Long-Baseline Neutrino Facility: Building the Future The Long-Baseline Neutrino Facility (LBNF) will be the world’s flagship science project to unlock the mysteries of neutrinos, the particles that could be the key to explaining why matter exists in our universe. It will house the infrastructure and particle detectors for the Deep Underground Neutrino Experiment (DUNE) and will use the world’s Sanford Fermi National most intense neutrino beam. LBNF will be hosted at the U.S. Depart- Underground Accelerator Research Facility, Laboratory, Illinois ment of Energy’s Fermi National Accelerator Laboratory in Illinois South Dakota and the Sanford Underground Research Facility in South Dakota. About 1,000 scientists from more than 160 laboratories and universities in 30 countries are contributing to this international mega-science project. In addition to direct economic benefits to the states of Illinois and South Dakota, LBNF will foster STEM education nationwide 800 miles/1300 km and keep the United States at the leading edge of global science and innovation. Learn more about the project and read the full economic impact report at lbnf.fnal.gov Economic impact, 2016-2026* South Dakota Illinois $952 million $340 million $1,204 million $593 million Total economic output Income for South Dakota Total economic output Income for Illinois households households 90% of economic output is in the 13-county western 94% of economic output is in the 9-county Chicago metro region South Dakota region Jobs created, 2016–2026* 2,500 2,084 1,859 1,500 Jobs in South Dakota Jobs in Illinois Year 2016 2020 2024 2026 *As each dollar spent on LBNF and DUNE enters the economy, it supports additional business activity, jobs and payroll. -
Construction of a Dust Detector for the Colorado Dust Accelerator
Construction of a Dust Detector for the Colorado Dust Accelerator Evan Thomas University of Colorado REU summer 2009 Introduction Since the Apollo years, lunar scientists have been left searching for explanations to anomalous dust transport on the surface of the Moon, given the lack of wind on the Moon’s surface. The Apollo 17 crew observed bright streams extending to about 100 km above the lunar surface. These observations were attributed to dust grains, on the order of ~0.1 μm, scattering sunlight [McCoy and Criswell, 1974; Zook and McCoy 1991]. Visual observations and photographs from the Clementine mission also indicated there is dust at high altitudes in the Moon’s exosphere (an exosphere is a very diffuse atmosphere), though there has been no definitive proof of this up to now. Further measurements on the lunar surface and remote sensing observations suggest that dusty plasma is responsible for the transport of grains from the surface [Criswell, 1973; Rennilson and Criswell, 1974]. Future missions like the Lunar Atmosphere and Dust Environment Explorer (LADEE) could shed light on the exosphere’s characteristics, but for these missions to be successful, a deeper understanding of the dynamics of this plasma and how it relates to dust transport is needed. This paper will describe current lunar models as well as describe an upcoming dust accelerator experiment, which hopes to uncover key parameters of these models, focusing on dust parameter detection. During the Moon’s orbit outside Earth’s magnetosphere, the surface is bombarded with Solar wind plasma and UV radiation. The side facing the sun becomes positively charged due to photoelectrons leaving the surface and escaping.