Combined Study of Reactor and Terrestrial Antineutrinos with Kamland
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Klinkenberg Effect on Predicting and Measuring Helium Permeability in Gas Shales
International Journal of Coal Geology 123 (2014) 62–68 Contents lists available at ScienceDirect International Journal of Coal Geology journal homepage: www.elsevier.com/locate/ijcoalgeo Klinkenberg effect on predicting and measuring helium permeability in gas shales Mahnaz Firouzi, Khalid Alnoaimi, Anthony Kovscek, Jennifer Wilcox ⁎ Department of Energy Resources Engineering, Stanford University, Stanford, CA 94305-2220, USA article info abstract Article history: To predict accurately gas-transport in shale systems, it is important to study the transport phenomena of a non- Received 21 June 2013 adsorptive gas such as helium to investigate gas “slippage”. Non-equilibrium molecular dynamics (NEMD) sim- Received in revised form 24 September 2013 ulations have been carried out with an external driving force imposed on the 3-D carbon pore network generated Accepted 24 September 2013 atomistically using the Voronoi tessellation method, representative of the carbon-based kerogen porous struc- Available online 1 October 2013 ture of shale, to investigate helium transport and predict Klinkenberg parameters. Simulations are conducted to determine the effect of pressure on gas permeability in the pore network structure. In addition, pressure Keywords: Klinkenberg pulse decay experiments have been conducted to measure the helium permeability and Klinkenberg parameters Molecular modeling of a shale core plug to establish a comparison between permeability measurements in the laboratory and the per- Measurement meability predictions using NEMD simulations. The results indicate that the gas permeability, obtained from Helium pulse-decay experiments, is approximately two orders of magnitude greater than that calculated by the MD sim- Permeability ulation. The experimental permeability, however, is extracted from early-time pressure profiles that correspond Shale to convective flow in shale macropores (N50 nm). -
CERN Celebrates Discoveries
INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 43 NUMBER 10 DECEMBER 2003 CERN celebrates discoveries NEW PARTICLES NETWORKS SPAIN Protons make pentaquarks p5 Measuring the digital divide pl7 Particle physics thrives p30 16 KPH impact 113 KPH impact series VISyN High Voltage Power Supplies When the objective is to measure the almost immeasurable, the VISyN-Series is the detector power supply of choice. These multi-output, card based high voltage power supplies are stable, predictable, and versatile. VISyN is now manufactured by Universal High Voltage, a world leader in high voltage power supplies, whose products are in use in every national laboratory. For worldwide sales and service, contact the VISyN product group at Universal High Voltage. Universal High Voltage Your High Voltage Power Partner 57 Commerce Drive, Brookfield CT 06804 USA « (203) 740-8555 • Fax (203) 740-9555 www.universalhv.com Covering current developments in high- energy physics and related fields worldwide CERN Courier (ISSN 0304-288X) is distributed to member state governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly, except for January and August, in English and French editions. The views expressed are CERN not necessarily those of the CERN management. Editor Christine Sutton CERN, 1211 Geneva 23, Switzerland E-mail: [email protected] Fax:+41 (22) 782 1906 Web: cerncourier.com COURIER Advisory Board R Landua (Chairman), P Sphicas, K Potter, E Lillest0l, C Detraz, H Hoffmann, R Bailey -
About Testing Nu Mu Oscillation with Dm2 Smaller Than 0.001 Ev2 With
2 About testing νµ oscillation with ∆m smaller than 0.001 eV2 with the CERN Proton Synchrotron P. F. Loverre, R. Santacesaria, F. R. Spada Universit`a“La Sapienza” and Istituto Nazionale di Fisica Nucleare (INFN) Rome, Italy – Submitted to The European Physical Journal C Abstract We study the feasibility of a long–baseline neutrino experiment from CERN to Gran Sasso LNGS Laboratories using the CERN PS accelerator. Baseline and neutrino energy spectrum are suitable to explore a region of the (∆m2, sin2 2θ) parameters space which is not reached by K2K, the first experiment that will test at accelerator the atmospheric neutrino anomaly put in evidence by Super–Kamiokande. The recent Super–Kamiokande measurements of atmospheric neutrino arXiv:hep-ex/9911043v1 29 Nov 1999 fluxes [1] favour νµ → ντ (or νµ → νx) oscillations, with almost maximal mixing and ∆m2 in the range (5 ÷ 60) · 10−4 eV2. The first test of this atmospheric neutrino anomaly at accelerator will be performed in Japan by the K2K [2] experiment. K2K has recently started taking data using a neutrino beam generated by the KEK 12–GeV Pro- ton Synchrotron directed toward the Super–Kamiokande detector, which is placed about 250 Km away from KEK. The K2K experiment, owing to an L/E ratio of order 250/1 (Km/GeV), explores via disappearance νµ oscilla- tions down to ∆m2 ∼ 2 · 10−3 eV2. The same ∆m2 region can be explored with higher sensitivity with the high energy neutrino beams of FNAL (NuMI – MINOS experiment [3,4]) and 1 CERN (CERN – Gran Sasso LNGS beam [5]). -
K2K Cross Section Studies
K2K Cross Section Studies Rik Gran U. Minnesota Duluth 0. K2K experiment and NEUT interaction code 1. NC single p0/(All CC) in 1KT Cherenkov detector 2. CC-Coherent Pion Production in SciBar detector 3. MA-QE from shape fit to SciFi detector data Motivations Improve Neutrino Cross Sections knowledge of Cross Sections (Lipari 1995) En (GeV) Cross Sections and Nuclear Effects are important for extracting oscillation parameters from nu-mu disappearance nu-e appearance experiments. K2K oscillation result K2K beamline at KEK in Tsukuba, Japan OperK2Kated frneutom ri1999no osci to 2004llation experiment Al target 12 GeV PS 200m fast extraction every 2.2sec beam spill width 1.1s ( 9 bunches ) ~6x1012 protons/spill K2K beam and near detectors 98% pure n beam target materials: H2O, HC, Fe n energies SciFi Water Target at the K2K near detectors En (GeV) The NEUT neutrino interaction model Charged current quasi-elastic n + N -> l + N' Neutral current elastic n + N -> n + N CC/NC single p (h,K) resonance n + N -> l(n) + N' + p NC coherent pion (not CC !) n + A -> n + A + p0 CC/NC deep inelastic scattering n + q -> l(n) + had Cross-sections Total (NC+CC) n = neutrino (e, or t) ) V CC Total e l = lepton (e, or t) G / 2 m c CC quasi-elastic 8 3 - 0 1 From 100 MeV to 10 TeV ( DIS E / CC single π (cosmic ray induced neutrinos too!) σ NC single π0 Eν (GeV) More about the interaction models Quasi-elastic follows Llewelyn-Smith using dipole form factors and MAQE = 1.1 GeV (For neutrino beam, target is always neutron) Resonance production from Rein and Sehgal 18 resonances, MA1p = 1.1 GeV (Coherent pion production also from Rein and Sehgal) Deep inelastic Scattering from GRV94 PYTHIA/JETSET for hadron final states Bodek-Yang correction in Resonance-DIS overlap region Description and references available in Ch. -
Carrier Dynamics in Single Luminescent Silicon Quantum Dots
Carrier Dynamics in Single Luminescent Silicon Quantum dots Fatemeh Sangghaleh PhD Thesis Information and Communication Technology KTH Royal Institute of Technology Stockholm, Sweden 2015 TRITA-ICT 2015:09 KTH School of Information and Communication Technology SE-164 40, ISBN 978-91-7595-665-7 Kista, SWEDEN A dissertation submitted to KTH Royal Institute of Technology, Stockholm, Sweden, in partial fulfillment of requirements for the degree of Teknologie Doktor (Doctor of Philosophy). The defense will take place on October 23 2015 at 10.00 a. m. at Sal C, KTH- Electrum, Kistagången 16, Kista. © Fatemeh Sangghaleh, October 2015. Printed by: Universitetsservice US-AB Abstract Bulk silicon as an indirect bandgap semiconductor is a poor light emitter. In contrast, silicon nanocrystals (Si NCs) exhibit strong emission even at room temperature, discovered initially at 1990 for porous silicon by Leigh Canham. This can be explained by the indirect to quasi-direct bandgap modification of nano-sized silicon according to the already well-established model of quantum confinement. In the absence of deep understanding of numerous fundamental optical properties of Si NCs, it is essential to study their photoluminescence (PL) characteristics at the single-dot level. This thesis presents new experimental results on various photoluminescence mechanisms in single silicon quantum dots (Si QDs). The visible and near infrared emission of Si NCs are believed to originate from the band-to-band recombination of quantum confined excitons. However, the mechanism of such process is not well understood yet. Through time-resolved PL decay spectroscopy of well-separated single Si QDs, we first quantitatively established that the PL decay character varies from dot-to-dot and the individual lifetime dispersion results in the stretched exponential decays of ensembles. -
April 2003 $4.95
SOLVING THE NEUTRINO MYSTERY • RECOGNIZING ANCIENT LIFE APRIL 2003 $4.95 WWW.SCIAM.COM James D.Watson discusses DNA, the brain, designer babies and more as he reflects on Grid Computing’s Unbounded Potential Ginkgo Biloba Will Mount Etna and Memory Explode Tomorrow? Delivering Drugs with Implanted Chips COPYRIGHT 2003 SCIENTIFIC AMERICAN, INC. april 2003 contentsSCIENTIFIC AMERICAN Volume 288 Number 4 features ASTROPHYSICS 40 Solving the Solar Neutrino Problem BY ARTHUR B. MCDONALD, JOSHUA R. KLEIN AND DAVID L. WARK After 30 years, physicists fathom the mystery of the missing neutrinos: the phantom particles change en route from the sun. BIOTECHNOLOGY 50 Where a Pill Won’t Reach BY ROBERT LANGER Implanted microchips, embedded polymers and ultrasonic blasts of proteins will deliver next-generation medicines. 66 James D. Watson VOLCANOLOGY 58 Mount Etna’s Ferocious Future BY TOM PFEIFFER Europe’s most active volcano grows more dangerous, but slowly. CELEBRATING THE GENETIC JUBILEE 66 A Conversation with James D. Watson The co-discoverer of DNA’s double helix reflects on the molecular model that changed both science and society. LIFE SCIENCE 70 Questioning the Oldest Signs of Life BY SARAH SIMPSON Researchers are reevaluating how they identify traces left by life in ancient rocks on earth—and elsewhere in the solar system. INFORMATION TECHNOLOGY 78 The Grid: Computing without Bounds BY IAN FOSTER Powerful global networks of processors and storage may end the era of self-contained computing. MEDICINE 86 The Lowdown on Ginkgo Biloba BY PAUL E. GOLD, LARRY CAHILL AND GARY L. WENK This herbal supplement may slightly improve your memory—but so can eating a candy bar. -
CERN Courier Is Distributed to Member-State Governments, Institutes and Laboratories Affiliated with CERN, and to Their Personnel
I n t e r n at I o n a l J o u r n a l o f H I g H - e n e r g y P H y s I c s CERN COURIERV o l u m e 4 6 n u m b e r 9 n o V e m b e r 2 0 0 6 OPERA makes its grand debut ACCELERATORS COMPUTING NEWS INTERVIEW Laser-wakefield device Business signs up to Stephen Hawking pays reaches 1 GeV p5 work with EGEE p12 a visit to CERN p28 CCENovCover1.indd 1 18/10/06 08:53:59 CERN & ProCurve Networking 15 petabytes of data And a network that can handle it “CERN uses ProCurve Switches because we generate a colossal amount of data, making dependability a top priority.” —David Foster, Communication Systems Group Leader, CERN CERN has joined with ProCurve to build their network based on high-performance security, reliability and flexibility, along with a lifetime warranty.* From the world’s largest applications, to a company-wide email, just think what ProCurve could do for your network. Get a closer look at CERN and the world’s biggest physics experiment. Visit www.hp.com/eur/procurvecern1 *For as long as you own the product, with next-business-day advance replacement (available in most countries). For details, refer to the ProCurve Software License, Warranty and Support booklet at www.hp.com/rnd/support/warranty/index.htm The ProCurve Routing Switch 9300m series, ProCurve Routing Switch 9408sl, ProCurve Switch 8100fl series, and the ProCurve Access Control Server 745wl have a one-year- warranty with extensions available. -
Long Baseline Neutrino Oscillation Experiments 1 Introduction 2
Long Baseline Neutrino Oscillation Experiments Mark Thomson Cavendish Laboratory Department of Physics JJ Thomson Avenue Cambridge, CB3 0HE United Kingdom 1 Introduction In the last ten years the study of the quantum mechanical e®ect of neutrino os- cillations, which arises due to the mixing of the weak eigenstates fºe; º¹; º¿ g and the mass eigenstates fº1; º2; º3g, has revolutionised our understanding of neutrinos. Until recently, this understanding was dominated by experimental observations of at- mospheric [1, 2, 3] and solar neutrino [4, 5, 6] oscillations. These measurements have been of great importance. However, the use of naturally occuring neutrino sources is not su±cient to determine fully the flavour mixing parameters in the neutrino sector. For this reason, many of the current and next generation of neutrino experiments are based on high intensity accelerator generated neutrino beams. The ¯rst generation of these long-baseline (LBL) neutrino oscillation experiments, K2K, MINOS and CNGS, are the main subject of this review. The next generation of LBL experiments, T2K and NOºA, are also discussed. 2 Theoretical Background For two neutrino weak eigenstates fº®; º¯g related to two mass eigenstates fºi; ºjg, by a single mixing angle θij, it is simple to show that the survival probability of a neutrino of energy Eº and flavour ® after propagating a distance L through the vacuum is à ! 2 2 2 2 1:27¢mji(eV )L(km) P (º® ! º®) = 1 ¡ sin 2θij sin ; (1) Eº(GeV) 2 2 2 where ¢mji is the di®erence of the squares of the neutrino masses, mj ¡ mi . -
Evolution of Helium with Temperature in Neutron-Irradiated 10 B-Doped
Hindawi Publishing Corporation Advances in Condensed Matter Physics Volume 2014, Article ID 506936, 6 pages http://dx.doi.org/10.1155/2014/506936 Research Article Evolution of Helium with Temperature in Neutron-Irradiated 10B-Doped Aluminum by Small-Angle X-Ray Scattering Chaoqiang Huang,1,2,3 Guanyun Yan,2,3 Qiang Tian,2,3 Guangai Sun,2,3 Bo Chen,2,3 Liusi Sheng,1 Yaoguang Liu,2,3 Xinggui Long,2,3 Xiao Liu,2,3 Luhui Han,4 and Zhonghua Wu5 1 College of Nuclear Science and Technology, University of Science and Technology of China, Hefei 230029, China 2 Institute of Nuclear Physics and Chemistry, China Academy of Engineering Physics, Mianyang 621900, China 3 Key Laboratory of Neutron Physics, China Academy of Engineering Physics, Mianyang 621900, China 4 China Academy of Engineering Physics, Mianyang 621900, China 5 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China Correspondence should be addressed to Chaoqiang Huang; [email protected] Received 28 February 2014; Revised 20 May 2014; Accepted 5 June 2014; Published 22 June 2014 AcademicEditor:Xiao-TaoZu Copyright © 2014 Chaoqiang Huang 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. 10 Helium status is the primary effect of material properties under radiation. B-doped aluminum samples were prepared via arc melting technique and rapidly cooled with liquid nitrogen to increase the boron concentration during the formation of compounds. 25 −3 10 An accumulated helium concentration of ∼6.2 × 10 m was obtained via reactor neutron irradiation with the reaction of B(n, 7 ) Li. -
Department of Energy National Science Foundation
Department of Energy National Science Foundation Report of Scientific Assessment Group on Experimental Non-Accelerator Physics (SAGENAP) March 12-14, 2002 Eugene Loh, NSF, Co-Chair James Stone, DoE, Co-Chair Steven Ritz, Report Coordinator SAGENAP Meeting Summary Report March 12-14, 2002 The Scientific Assessment Group for Experiments in Non-Accelerator Physics (SAGENAP) met on March 12-14, 2002, in Ballston, VA at the Arlington Hilton, with NSF as the host agency. The group members for this meeting were Janet Conrad (Columbia), Priscilla Cushman (Minnesota), Jordan Goodman (Maryland), Giorgio Gratta (Stanford), Francis Halzen (Wisconsin), James Musser (Indiana), Rene Ong (UCLA), Steven Ritz (Goddard), Hamish Robertson (U. of Washington), Robert Svoboda (Louisiana State), James Yeck (DoE), James Stone (DoE), and Eugene Loh (NSF). The meeting was co-chaired by Eugene Loh and James Stone, with Steven Ritz serving as report coordinator. Janet Conrad was absent from this meeting. Jordan Goodman and Hamish Robertson left the meeting early. Five proposals were considered at this meeting: XENON, OMNIS, 3M, Super- Kamiokande repair, and Solar Neutrino TPC. Written versions of the proposals were available to members of SAGENAP. The proponents made oral presentations during the meeting (see the Appendix for the agenda), followed by questions and answers with the group members. Individual written reviews of the proposals by SAGENAP members have been provided to the DoE and NSF. At least four individual reviews by different SAGENAP members were written for each proposal. Two additional projects were considered: the Nearby Supernova Factory, based at LBNL, and a Letter of Intent for further work on ICARUS. -
Results from the K2K Experiment
Results from the K2K experiment T. Nakadaira KEK 1 K2K experiment lKEK to Kamioka long baseline Neutrino Oscillation Experiment 250km áEnñ~1.3GeV Super-Kamiokande Far Detector Fiducial vol. : 22.5kt KEK 12GeV PS n beam line Near Detector(ND) Started in 1999 2 K2KK2K CollaborationCollaboration JAPAN: High Energy Accelerator Research Organization (KEK) / Institute for Cosmic Ray Research (ICRR), Univ. of Tokyo / Kobe University / Kyoto University / Niigata University / Okayama University / Tokyo University of Science / Tohoku University KOREA: Chonnam National University / Dongshin University / Korea University / Seoul National University U.S.A.: Boston University / University of California, Irvine / University of Hawaii, Manoa / Massachusetts Institute of Technology / State University of New York at Stony Brook / University of Washington at Seattle POLAND: Warsaw University / Solton Institute Since 2002 JAPAN: Hiroshima University / Osaka University CANADA: TRIUMF / University of British Columbia ITALY: Rome FRANCE: Saclay SPAIN: Barcelona / Valencia SWITZERLAND: Geneva RUSSIA: INR-Moscow U.S.A.: Duke University 3 Principle of K2K 11 12GeV protons ~10 nm/2.2sec ~1 event/2days (/10m´10m) nm + p m+ SK nt Target+Horn 200m 100m ~250km decay pipe p monitor Near n detectors m monitor 2 2 2 1.27Dm L •Confirmation of n àn oscillation prob.=×sin2q sin() m x E reported by Super-K atm-n n nm spectrum@SK Observables: For Dm2=3x10-3, 2 lReduction of events sin 2q=1 lDistortion of spectrum à If sin22q¹0 and Dm2¹0, Neutrino oscillation. En [GeV]4 Neutrino -
History of Long-Baseline Accelerator Neutrino Experiments∗
History of Long-Baseline Accelerator Neutrino Experiments∗ Gary J. Feldman Department of Physics, Harvard University, 17 Oxford Street, Cambridge, MA 02138, United States I will discuss the six previous and present long-baseline neutrino experiments: two first- generation general experiments, K2K and MINOS, two specialized experiments, OPERA and ICARUS, and two second-generation general experiments, T2K and NOνA. The motivations for and goals of each experiment, the reasons for the choices that each experiment made, and the outcomes will be discussed. 1 Introduction My assignment in this conference is to discuss the history of the six past and present long- baseline neutrino experiments. Both Japan and the United States have hosted first- and second- generation general experiments, K2K and T2K in Japan and MINOS and NOνA in the United States. Europe hosted two more-specialized experiments, OPERA and ICARUS. Since the only possible reason to locate a detector hundreds of kilometers from the neutrino beam target is to study neutrino oscillations, the discussion will be limited to that topic, although each of these experiments investigated other topics. Also due to the time limitation, with one exception, I will not discuss sterile neutrino searches. These experiment have not found any evidence for sterile neutrinos to date.1;2;3;4;5;6;7 The Japanese and American hosted experiments have used the comparison between a near and far de- tector to measure the effects of oscillations. This is an essential method of reducing systematic uncertain- ties, since uncertainties due flux, cross sections, and efficiencies will mostly cancel. The American experi- ments used functionally equivalent near detectors and the Japanese experiments used detectors that were func- tionally equivalent, fine-grained, or both.