Christopher Williams, Ph.D.
|
|
- Alexis Hensley
- 6 years ago
- Views:
Transcription
1 Senior Associate Statistical & Data Sciences 149 Commonwealth Drive Menlo Park, CA (650) tel Professional Profile Dr. Williams specializes in the implementation and evaluation of information assurance and data collection techniques to solve emerging problems around transaction security and privacy in the Internet of things (IoT), financial technology ("fintech"), transportation, and Intelligence. Dr. Williams has diverse scientific experience with expertise in applied cryptography, solutions engineering, systems integration, instrumentation, experimental design, and real-time data acquisition with a focus on systematic error mitigation. He has applied his expertise to validate standards compliance in secure messaging protocols between a smart card and host; and to study the integration of commercial encryption solutions into a government approved authentication infrastructure for mobile platforms. Dr. Williams has a Ph.D. in Physics from University of Chicago, where his dissertation research focused on design, prototyping, and field deployment of novel detectors for particle astrophysics. This included full life-cycle development of an ultra-fast, ultra-wide field imaging microwave telescope which combined consumer off-the-shelf hardware with custom digitizing electronics for triggering and data acquisition. He also has extensive experience in beam test and radioactive environments performing single-photon UV and microwave measurements. Prior to joining Exponent, Dr. Williams had a postdoctoral position as a Kavli Fellow at the Kavli Institute for Particle Astrophysics and Cosmology of Stanford University and SLAC National Accelerator Laboratory. His work focused on system design and integration of superconducting quantum detectors for large-scale x-ray spectrometers to be used in space telescopes and terrestrial x-ray source measurements. Dr. Williams is a founding member of the Secure Technology Alliance's IoT Security Council and serves on the Federal Reserve's Secure Payments Task Force. Academic Credentials & Professional Honors Ph.D., Physics, University of Chicago, 2013 M.S., Physics, University of Chicago, 2009 B.S., Astronomy & Physics, The Ohio State University, magna cum laude, with honors, with research distinction in physics, 2008 Kavli Fellowship, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University (2013) Dr. Pliny A. & Margaret H. Price Prize, Center for Cosmology and Astro-Particle Physics, The Ohio State University (2012) 09/17 Page 1
2 Gaurang & Kanwal Yodh Prize, Department of Physics, University of Chicago (2012) Selected as a Young Researcher participant of the 62nd Lindau Nobel Laureate Meeting, Lindau, Germany (July 2012) Albert A. Michelson Fellowship, Department of Physics, University of Chicago ( ) Eugene and Niesje Parker Fellowship, Department of Physics, University of Chicago; ( ) Robert G. Sachs Fellowship, Department of Physics, University of Chicago ( ) Smith Senior Award, Department of Physics, The Ohio State University (2008) Licenses and Certifications Offensive Security Wireless Professional, 2016, #OS-BWA Publications Belov K., et al. Accelerator measurements of magnetically induced radio emission from particle cascades with applications to cosmic-ray air showers. Physical Review Letters 2016; 116: Alvarez-Muñiz J, et al. The MIDAS telescope for microwave detection of ultra-high publications energy cosmic rays. Nuclear Instruments and Methods in Physics Research Section A 2013; 719:70. Ave M, et al. Precise measurement of the absolute uorescence yield of the 337 nm band in atmospheric gases. Astroparticle Physics 2013; 42:90. Alvarez-Muñiz J, et al. (Williams, C. Corresponding Author). Search for microwave emission from ultrahigh energy cosmic rays. Physical Review D 2012; 86:051104(R). Williams C. (for The Pierre Auger Collaboration). Microwave detection of cosmic ray air showers at the Pierre Auger Observatory, an R&D effort. Physics Procedia 2012; 37:1341. Gorham PW, et al. The Antarctic Impulsive Transient Antenna ultra-high energy neutrino detector: Design, performance, and sensitivity for the balloon flight. Astroparticle Physics 2009; 32:10. Invited Talks Williams C. Future challenges in understanding ultra-high energy cosmic rays. NASA Goddard Spaceight Center, Greenbelt, MD, USA, December Williams C. Isotropic microwave emission from extensive air showers. Multi-messenger Approaches to Cosmic Rays: Origins and Space frontiers, Institut d'astrophysicque de Paris, France, November Williams C. The MIDAS telescope. KIPAC Tea Talk, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Palo Alto, CA, USA, January Williams C. Microwave transient telescopes: Cosmic rays and beyond. SETI Institute, Mountain View, CA, USA, January Williams C. Microwave detection of cosmic ray air showers. NPAC Forum, Department of Physics, University of Wisconsin, Madison, WI, USA, November /17 Page 2
3 Williams C. Microwave detection of cosmic ray air showers. Price Prize Lecture, Center for Cosmology and AstroParticle Physics, The Ohio State University, Columbus, OH, USA, October Williams C. Ultra-high energy cosmic rays. 220th AAS Meeting, Anchorage, AK, USA, June Williams C. Microwave Detection of Air Showers (MIDAS): A Path Under Experiment. TAPIR Seminar, California Institue of Technology, Pasadena, CA, USA, April 2012 Proceedings Williams C, et al. First results from the Microwave Air Yield Beam Experiment (MAYBE): Measurement of GHz radiation of ultra-high energy cosmic ray detection. Proceedings, International Symposium on Future Directions in UHECR Physics, EPJ Web of Conferences 53, 08008, Bogdan M, et al. Front-end electronics and data acquisition system for the MIDAS experiment IEEE Nuclear Science Symposium, Conference Record, pp , NP3.M-114, Valencia, Spain, October 23-29, Monasor M, et al. The Microwave Air Yield Beam Experiment (MAYBE): Measurement of GHz radiation for ultra-high energy cosmic rays detection. Proceedings, 32nd International Cosmic Ray Conference, The Pierre Auger Collaboration (Presentation by P. Allison). Microwave detection of cosmic ray showers at the Pierre Auger Observatory. Proceedings, 32nd International Cosmic Ray Conference, Privitera P, et al. Microwave detection of air showers with the MIDAS experiment. Nuclear Physics B - Proceedings Supplements 2011; : 329. Ave M, et al. (AIRFLY Collaboration). Precise measurement of the absolute yield of fluorescence photons in atmospheric gases. Nuclear Physics B - Proceedings Supplements 2011; :361. Ave M, et al. (AIRFLY Collaboration). Precise measurement of the absolute fluorescence yield. International Symposium on the Recent Progress Of Ultra-High Energy Cosmic Ray Observation, AIP Conference Proceedings 2010; 1367, 29. Williams C, et al. The MIDAS Experiment: A new technique for the detection of extensive air showers. Proceedings, XVI International Symposium on Very High Energy Cosmic Ray Interactions, Conference Presentations Williams C. The MIDAS Telescope for the detection of ultra-high energy cosmic rays. URSI Meeting, Boulder, CO, USA, January Williams C. New detection techniques for ultra-high energy cosmic rays, an R&D effort for wide-field microwave transient telescopes. CASPER Workshop, Green Bank, WV, USA, August Williams C, et al. The Microwave Air Yield Beam Experiment (MAYBE): Measurement of GHz radiation for ultra-high energy cosmic rays detection. American Physical Society April Meeting, Atlanta, GA, USA, April Williams C, et al. First results from the Microwave Air Yield Beam Experiment (MAYBE): Measurement of GHz radiation of ultra-high energy cosmic ray detection. International Symposium on Future Directions in UHECR Physics, CERN, Geneva, Switzerland, February /17 Page 3
4 Williams C, for The Pierre Auger Collaboration. Microwave detection of cosmic ray air showers at the Pierre Auger Observatory, an R&D effort. Technology and Instrumentation in Particle Physics 2011, Chicago, IL, USA, June Williams C. Laser calibration of the AIRFLY experiment. 7th Air Fluorescence Workshop, Coimbra, Portugal, September Williams C, et al. The MIDAS Experiment: A new technique for the detection of extensive air showers. XVI International Symposium on Very High Energy Cosmic Ray Interactions, Batavia, IL, USA, June Williams C. Absolute calibration of PMTs with Rayleigh Scattered Laser Light. 6th Air Fluorescence Workshop, L'Aquila, Italy, February Collaboration Publications The Pierre Auger Collaboration. Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America. Atmospheric Research 2014; 149:120. The Pierre Auger Collaboration. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications. Physical Review D 2014; 90(12): The Pierre Auger Collaboration. Depth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above 1017:8 ev. Physical Review D 2014; 90(12). The Pierre Auger Collaboration. Searches for large-scale anisotropy in the arrival directions of cosmic rays detected above energy of 1019 ev at the Pierre Auger Observatory and the Telescope Array. The Astrophysical Journal 2014; 794(2):172. The Pierre Auger Collaboration. Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth. Physical Review D 2014; 90(1): The Pierre Auger Collaboration. A targeted search for point sources of EeV neutrons. The Astrophysical Journal Letters 2014; 789(2): L34. The Pierre Auger Collaboration. A search for point sources of EeV photons. Astrophysical Journal 2014; 789(2):160. The Pierre Auger Collaboration. Probing the radio emission from air showers with polarization measurements. Physical Review D 2014; 89(5): The Pierre Auger Collaboration. Identifying clouds over the Pierre Auger Observatory using infrared satellite data. Astroparticle Physics 2013; 50(92). The Pierre Auger Collaboration. Ultra-high energy neutrinos at the Pierre Auger Observatory. Advances in High Energy Physics 2013; The Pierre Auger Collaboration. The interpretation of the depths of shower maximum of extensive air showers measured by the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics 2013; 02:026. The Pierre Auger Collaboration. Constraints on the origin of cosmic rays above 1018 ev from large scale anisotropy searches in data of the Pierre Auger observatory. Astrophysical Journal Letters 2013; 762:L13. The Pierre Auger Collaboration. Large scale distribution of arrival directions of cosmic rays detected above 1018 ev at the Pierre Auger observatory. Astrophysical Journal Supplement 2012; 203:34. 09/17 Page 4
5 The Pierre Auger Collaboration. A search for point sources of EeV Neutrons. Astrophysical Journal 2012; 760:148. The Pierre Auger Collaboration. Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory. Journal of Instrumentation The Pierre Auger Collaboration. Ultra-high energy neutrinos at the Pierre Auger Observatory. Advances in High Energy Physics The Pierre Auger Collaboration. The rapid atmospheric monitoring system of the Pierre Auger Observatory. Journal of Instrumentation 2012; 7:P The Pierre Auger Collaboration. Measurement of the proton-air cross-section at P s = 57 TeV with the Pierre Auger Observatory. Physical Review Letters 2012; 109: The Pierre Auger Collaboration. Search for point-like sources of ultra-high energy neutrinos at the Pierre Auger Observatory and improved limit on the diffuse ux of tau neutrinos. Astrophysical Journal Letters 2012; 755:L4. The Pierre Auger Collaboration. A search for anisotropy in the arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics 2012; 04:040. The Pierre Auger Collaboration. Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS). Astroparticle Physics 2012; 35:591. The Pierre Auger Collaboration. Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory. Astroparticle Physics 2012; 35:354. The Pierre Auger Collaboration. Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory. Physical Review D 2011; 84: The Pierre Auger Collaboration. The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics 2011; 11:022. The Pierre Auger Collaboration. The lateral trigger probability function for UHE cosmic rays showers detected by the Pierre Auger Observatory. Astroparticle Physics 2011; 35:266. The Pierre Auger Collaboration. Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory. Journal of Cosmology and Astroparticle Physics 2011; 06:022. The Pierre Auger Collaboration. Advanced functionality for radio analysis in the Offine software framework of the Pierre Auger Observatory. Nuclear Instruments and Methods in Physics Research 2011; A635:92. The Pierre Auger Collaboration. Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory. Astroparticle Physics 2011; 34:627. The Pierre Auger Collaboration. The Pierre Auger Observatory scaler mode for the study of the modulation of galactic cosmic rays due to solar activity. Journal of Instrumentation 2011; 6:P The Pierre Auger Collaboration. The exposure of the hybrid detector of the Pierre Auger Observatory. 09/17 Page 5
6 Astroparticle Physics 2011; 34:368. The Pierre Auger Collaboration. Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter. Astroparticle Physics 2010; 34:314. The Pierre Auger Collaboration. The northern site of the Pierre Auger Observatory. New Journal of Physics 2010; 12: The Pierre Auger Collaboration. Measurement of the depth of maximum of extensive air showers above 1018 ev. Physical Review Letters 2010; 104: The Pierre Auger Collaboration. Measurement of the energy spectrum of cosmic rays above 1018 ev using the Pierre Auger Observatory. Physics Letters B 2010; 685:239. The Pierre Auger Collaboration. Trigger and aperture of the surface detector array of the Pierre Auger Observatory. Nuclear Instruments and Methods in Physics Research A 2010; 613:29. Conference Posters Williams C, et al. Microwave Detection of Air Showers (MIDAS). Centenary Symposium 2012: Discovery of Cosmic Rays, Denver, CO, USA, June Williams C, et al. The MIDAS Experiment, instrument design and first limits on ultra-high energy cosmic ray emission in microwaves. Wilhelm und Else Heraeus Seminar: Radio Detection in Astroparticle Physics, Bad Honnef, Germany, October /17 Page 6
Publications of Francesco Arneodo: journal articles
Publications of Francesco Arneodo: journal articles Figure 1: Citation report from ISI Web of Science (IF=31.0) [1] E. Aprile et al., First Axion Results from the XENON100 Experiment, arxiv.org (submitted
More informationDetecting High Energy Cosmic Rays with LOFAR
Detecting High Energy Cosmic Rays with LOFAR Andreas Horneffer for the LOFAR-CR Team LOFAR CR-KSP: Main Motivation Exploring the sub-second transient radio sky: Extensive Air showers as guaranteed signal
More informationWhat we (don t) know about UHECRs
What we (don t) know about UHECRs We know: their energies (up to 10 20 ev). their overall energy spectrum We don t know: where they are produced how they are produced what they are made off exact shape
More informationUltra- high energy cosmic rays
Ultra- high energy cosmic rays Tiina Suomijärvi Institut de Physique Nucléaire Université Paris Sud, Orsay, IN2P3/CNRS, France Atélier CTA, IAP, Paris, 30-31 June 2014 Outline Pierre Auger Observatory:
More informationThe Pierre Auger Observatory Status - First Results - Plans
The Pierre Auger Observatory Status - First Results - Plans Andreas Haungs for the Pierre Auger Collaboration Forschungszentrum Karlsruhe Germany haungs@ik.fzk.de Andreas Haungs Pierre Auger Observatory
More informationBrian Baughman Washington D.C
Washington D.C. 20001 http://umdgrb.umd.edu/~bbaugh/ OBJECTIVE Find a stimulating, diverse and stimulating work environment where I can leverage my skills to the benefit of science, students and thus humanity.
More informationRECENT RESULTS FROM THE PIERRE AUGER OBSERVATORY
RECENT RESULTS FROM THE PIERRE AUGER OBSERVATORY (Neutrino 2008, Christchurch, NZ) Esteban Roulet (Bariloche) the Auger Collaboration: 17 countries, ~100 Institutions, ~400 scientists Argentina, Australia,
More informationMass Composition Study at the Pierre Auger Observatory
OBSERVATORY Mass Composition Study at the Pierre Auger Observatory Laura Collica for the Auger Milano Group 4.04.2013, Astrosiesta INAF Milano 1 Outline The physics: The UHECR spectrum Extensive Air Showers
More informationUHE Cosmic Rays in the Auger Era
Vulcano Workshop 2010 - May, 23-29, 2010 UHE Cosmic Rays in the Auger Era Sergio Petrera, L'Aquila University email: sergio.petrera@aquila.infn.it Vulcano Workshop 2010 - May, 23-29, 2010 UHE Cosmic Rays
More informationStudy of the arrival directions of ultra-high-energy cosmic rays detected by the Pierre Auger Observatory
Study of the arrival directions of ultra-high-energy cosmic rays detected by the Pierre Auger Observatory Piera L. Ghia*, for the Pierre Auger Collaboration * IFSI/INAF Torino, Italy, & IPN/CNRS Orsay,
More informationNeutrino Astronomy fast-forward
Neutrino Astronomy fast-forward Marek Kowalski (DESY & Humboldt University Berlin) TeVPA 2017, Columbus, Ohio Credit: M. Wolf/NSF The promised land The Universe is opaque to EM radiation for ¼ of the spectrum,
More informationJohn Ellison University of California, Riverside. Quarknet 2008 at UCR
Cosmic Rays John Ellison University of California, Riverside Quarknet 2008 at UCR 1 What are Cosmic Rays? Particles accelerated in astrophysical sources incident on Earth s atmosphere Possible sources
More informationUltrahigh Energy cosmic rays II
Ultrahigh Energy cosmic rays II Today we will discuss the new data on UHECR presented during the last couple of years by the Auger observatory in Argentina. These data do not match previous analyses and
More information8. The Review of Particle Physics, K. Nakamura et al. (Particle Data Group), Phys. G 37, (2010).
Lawrence Wiencke Publications (Last Updated Sept 20 th 2011) Refereed Journals 1. The Lateral Trigger Probability function for UHE Cosmic Rays Showers detected by the Pierre Auger Observatory, J.Abraham
More informationStatus and results from the Pierre Auger Observatory
April 15-19, 2007 Aspen, Colorado Status and results from the Pierre Auger Observatory Lorenzo Perrone for the Auger Collaboration Università del Salento and INFN Lecce Italy The Physics Case: highest
More informationUltra-High Energy Cosmic Rays and Astrophysics. Hang Bae Kim Hanyang University Hangdang Workshop,
Ultra-High Energy Cosmic Rays and Astrophysics Hang Bae Kim Hanyang University Hangdang Workshop, 2012. 08. 22 Ultra High Energy Cosmic Rays Ultra High Energy Cosmic Ray (UHECR)» E 3 E & 10 18 ev Energy
More informationThe path towards measuring Cosmic Ray Air Showers from Space
The path towards measuring Cosmic Ray Air Showers from Space Francesca Bisconti KSETA Workshop 2017 13-15 February 2017 - Durbach KIT The Research University in the Helmholtz Association www.kit.edu Outline
More informationAn Auger Observatory View of Centaurus A
An Auger Observatory View of Centaurus A Roger Clay, University of Adelaide based on work particularly done with: Bruce Dawson, Adelaide Jose Bellido, Adelaide Ben Whelan, Adelaide and the Auger Collaboration
More informationTHE PIERRE AUGER OBSERVATORY: STATUS AND RECENT RESULTS
SF2A 2006 D. Barret, F. Casoli, T. Contini, G. Lagache, A. Lecavelier, and L. Pagani (eds) THE PIERRE AUGER OBSERVATORY: STATUS AND RECENT RESULTS Serguei Vorobiov (for the Pierre Auger Collaboration)
More informationDr. John Kelley Radboud Universiteit, Nijmegen
arly impressive. An ultrahighoton triggers a cascade of particles mulation of the Auger array. The Many Mysteries of Cosmic Rays Dr. John Kelley Radboud Universiteit, Nijmegen Questions What are cosmic
More informationAn introduction to AERA. An Introduction to the Auger Engineering Radio Array (AERA)
An Introduction to the Auger Engineering Radio Array (AERA) Amin Aminaei 1 for the Pierre Auger Collaboration 2,3 Abstract The new generation of radio-telescope arrays with digital interferometry is able
More informationThe ExaVolt Antenna (EVA)
The ExaVolt Antenna (EVA) Amy Connolly (Ohio State University) for the EVA collaboration University of Hawaii, OSU, George Washington University, NASA: JPL and Balloon Program Office Aspen Institute Feb.
More informationResults of the Search for Ultra High-Energy Neutrinos with ANITA-II
Results of the Search for Ultra High-Energy Neutrinos with ANITA-II Abby Goodhue Vieregg for the ANITA Collaboration University of California, Los Angeles 25 March 2010 (ANITA-II Launch Day in Antarctica)
More informationShort review and prospects of radio detection of high-energy cosmic rays. Andreas Haungs
Short review and prospects of radio detection of high-energy cosmic rays 1 To understand the sources of cosmic rays we need to know their arrival direction energy and mass we need large statistics large
More informationCosmic Rays - in Poland
Cosmic Rays - in Poland Maria Giller - University of Łódź Institutions: 1. Institute of Nuclear Physics Kraków, 2. University of Łódź, 3. Andrzej Sołtan Institute for Nuclear Studies - - Cosmic Ray group
More informationExtremely High Energy Neutrinos
Extremely High Energy Neutrinos A. Ringwald http://www.desy.de/ ringwald DESY 6 th National Astroparticle Physics Symposium February 3, 2006, Vrije Universiteit, Amsterdam, Netherlands Extremely high energy
More informationUltra-short Radio Pulses from High Energy Cosmic Rays
Ultra-short Radio Pulses from High Energy Cosmic Rays Andreas Horneffer for the LOFAR CR-KSP High Energy Cosmic Rays high energy particles dominated by atomic nuclei similar in composition to solar system
More informationLatest results and perspectives of the KASCADE-Grande EAS facility
Latest results and perspectives of the KASCADE-Grande EAS facility 29/6-2/7/2010, Nantes, France Andreas Haungs 1 Motivation KASCADE-Grande Knee EeV PeV g-eg? Radio?! KASCADE 10 15-10 17 ev: Origin of
More informationUHE Cosmic Rays and Neutrinos with the Pierre Auger Observatory
UHE Cosmic Rays and Neutrinos with the Pierre Auger Observatory Gonzalo Parente Bermúdez Universidade de Santiago de Compostela & IGFAE for the Pierre Auger Collaboration Particle Physics and Cosmology
More informationExperimental High-Energy Astroparticle Physics
KIT University of the State of Baden-Württemberg and National Research Center of the Helmholtz Association Experimental High-Energy Astroparticle Physics Andreas Haungs haungs@kit.edu 3 Content: 1. Introduction
More informationThe Tunka-Rex Experiment for the Detection of the Air- Shower Radio Emission
The Tunka-Rex Experiment for the Detection of the Air- Shower Radio Emission a) Y. Kazarina 1, P.A. Bezyazeekov 1, N.M. Budnev 1, O.A. Gress 1, A. Haungs 2, R.Hiller 2, T. Huege 2, M. Kleifges 3, E.N.
More informationSecondary particles generated in propagation neutrinos gamma rays
th INT, Seattle, 20 Feb 2008 Ultra High Energy Extragalactic Cosmic Rays: Propagation Todor Stanev Bartol Research Institute Dept Physics and Astronomy University of Delaware Energy loss processes protons
More informationResults from the Pierre Auger Observatory. Paul Sommers, Penn State August 7, 2008, SSI
Results from the Pierre Auger Observatory Paul Sommers, Penn State August 7, 2008, SSI The Cosmic Ray Energy Spectrum Non-thermal, approximate power law, up to about 3x10 20 ev (possibly higher) 1 EeV
More informationResults from the Pierre Auger Observatory
Thirteenth Marcel Grossmann Meeting - MG13 Stockholm, July 1-7, 2012 Results from the Pierre Auger Observatory Ivan De Mitri Università del Salento and INFN - Lecce, Italy for the Pierre Auger Collaboration
More informationVita Davison E. Soper
Vita Davison E. Soper Title: Professor, Department of Physics Address: Institute of Theoretical Science University of Oregon Eugene, Oregon 97403-5203 Phone Number: (541) 346-5162 Education: B.A., Amherst
More informationActivities of the Karlsruhe Center Elementary Particle and Astroparticle Physics (KCETA)
Activities of the Karlsruhe Center Elementary Particle and Astroparticle Physics (KCETA) Marc Weber KIT The Research University in the Helmholtz Association www.kit.edu fields particles collisions 2 Tradition
More informationAnisotropy studies with the Pierre Auger Observatory
Anisotropy studies with the Pierre Auger Observatory Carla Macolino 1 for the Pierre Auger Collaboration 2 Full author list: http://www.auger.org/archive/authors_2011_05.html 1 Lab. de Physique Nucleaire
More informationCurriculum Vitae Duncan L. Carlsmith
February 2012 Curriculum Vitae Duncan L. Carlsmith Contact information Dept. of Physics, 1150 University Ave, Madison, WI 53706 (608) 262-2485 (WI office), (608) 263-0800 (WI FAX), +41 79 233 34 98 (Swiss
More informationTopic 7. Relevance to the course
Topic 7 Cosmic Rays Relevance to the course Need to go back to the elemental abundance curve Isotopes of certain low A elements such as Li, Be and B have larger abundances on Earth than you would expect
More informationThe AUGER Experiment. D. Martello Department of Physics University of Salento & INFN Lecce. D. Martello Dep. of Physics Univ. of Salento & INFN LECCE
The AUGER Experiment D. Martello Department of Physics University of Salento & INFN Lecce The Pierre Auger Collaboration Argentina Australia Bolivia Brazil Croatia Czech Rep. France Germany Italy Mexico
More informationExtensive Air Showers and Particle Physics Todor Stanev Bartol Research Institute Dept Physics and Astronomy University of Delaware
Extensive Air Showers and Particle Physics Todor Stanev Bartol Research Institute Dept Physics and Astronomy University of Delaware Extensive air showers are the cascades that develop in the atmosphere
More informationCSSP14, Sinaia, 25 th July, Space-atmospheric interactions of ultra-high energy. cosmic rays. Gina Isar
CSSP14, Sinaia, 25 th July, 2014 Space-atmospheric interactions of ultra-high energy Gina Isar isar@spacescience.ro cosmic rays Outline Outline Cosmic rays: particles from outer space Earth is subject
More informationULTRA HIGH ENERGY COSMIC RAYS
ULTRA HIGH ENERGY COSMIC RAYS Carla Bonifazi Instituto de Física Universidade Federal do Rio de Janeiro Dark Side Of The Universe 2012 Buzios Brazil Outline Introduction UHECRs Detection Recent Progress
More informationSTUDY OF EXTENSIVE AIR SHOWERS IN THE EARTH S ATMOSPHERE
STUDY OF EXTENSIVE AIR SHOWERS IN THE EARTH S ATMOSPHERE I. BACIOIU * Institute of Space Science, P.O. Box MG-23, RO-077125 Bucharest-Magurele, Romania, E-mail: iuliana.bacioiu@spacescience.ro Abstract.
More information(High-Energy) Cosmic Rays
APPEC Town Meeting Roadmap ( Considerations ) Discussion (High-Energy) Cosmic Rays Paris, 6-7 April 2016 Andreas Haungs Karlsruhe Institute of Technology Petr Tinyakov Université Libre de Bruxelles petr.tiniakov@ulb.ac.be
More informationMatt Kistler Ohio State University In collaboration with John Beacom
Prospects for Galactic TeV Neutrino Astronomy Matt Kistler Ohio State University In collaboration with John Beacom Photo: HESS Zwicky s Contributions to GLCW8 COSMIC RA YS FROM SUPER-NO VAE By W. BAADE
More informationParameters Sensitive to the Mass Composition of Cosmic Rays and Their Application at the Pierre Auger Observatory
WDS'12 Proceedings of Contributed Papers, Part III, 137 141, 2012. ISBN 978-80-7378-226-9 MATFYZPRESS Parameters Sensitive to the Mass Composition of Cosmic Rays and Their Application at the Pierre Auger
More informationStatus and Perspectives of the LAGO Project
Status and Perspectives of the LAGO Project 5 th Workshop on Air Shower Detection at High Altitude Paris, France Édgar F. Carrera ecarrera@usfq.edu.ec (for the LAGO Collaboration) Universidad San Francisco
More informationProf. Rasha Abbasi. University of Utah Physics Department 115 South 1400 East Rm#201 Phone: +1 (801)
Prof. Rasha Abbasi Address University of Utah Physics Department 115 South 1400 East Rm#201 Phone: +1 (801) 808-1287 Salt Lake City UT 84112 E-mail: rasha@cosmic.utah.edu Position 2018-Now Research Assistant
More informationCurriculum Vitae. Reader-F: Institute of Physics, Bhubaneswar (Oct till date)
Curriculum Vitae Employment Reader-F: Institute of Physics, Bhubaneswar (Oct 2015 - till date) Fellow: Deutsches Elektronen-Synchrotron - DESY, Hamburg, Germany (Feb 2014 - Oct 2015) Post-doc: Institute
More informationStudies of Ultra High Energy Cosmic Rays with the Pierre Auger Observatory
Studies of Ultra High Energy Cosmic Rays with the Pierre Auger Observatory Universidade Federal do Rio de Janeiro, Brazil E-mail: haris@if.ufrj.br Aquiring data continuously from 004, the Pierre Auger
More informationIceCube. francis halzen. why would you want to build a a kilometer scale neutrino detector? IceCube: a cubic kilometer detector
IceCube francis halzen why would you want to build a a kilometer scale neutrino detector? IceCube: a cubic kilometer detector the discovery (and confirmation) of cosmic neutrinos from discovery to astronomy
More informationDevelopment of a prototype for Fluorescence detector Array of Single-pixel Telescopes (FAST)
Development of a prototype for Fluorescence detector Array of Single-pixel Telescopes (FAST) T. Fujii 1,2, P. Privitera 1, J. Jiang 1 construction is still, A. Matalon 1 in development, P. Motloch 1, M.
More informationUltrahigh Energy Cosmic Rays propagation II
Ultrahigh Energy Cosmic Rays propagation II The March 6th lecture discussed the energy loss processes of protons, nuclei and gamma rays in interactions with the microwave background. Today I will give
More informationGAMMA-RAY ASTRONOMY: IMAGING ATMOSPHERIC CHERENKOV TECHNIQUE FABIO ZANDANEL - SESIONES CCD
GAMMA-RAY ASTRONOMY: IMAGING ATMOSPHERIC CHERENKOV TECHNIQUE COSMIC RAYS Discovered in 1912 by Victor Hess (Nobel Prize) Messengers from the non-thermal part of the Universe E < 15 ev: galactic E > 17
More information7 th International Workshop on New Worlds in Astroparticle Physics São Tomé, September 2009 THE AMIGA PROJECT
7 th International Workshop on New Worlds in Astroparticle Physics São Tomé, 08 10 September 2009 THE AMIGA PROJECT P. GONÇALVES, M. PIMENTA, E. DOS SANTOS, B. TOMÉ LIP S. Tomé, 8 th September 2009 OUTLINE
More informationCosmic Rays. M. Swartz. Tuesday, August 2, 2011
Cosmic Rays M. Swartz 1 History Cosmic rays were discovered in 1912 by Victor Hess: he discovered that a charged electroscope discharged more rapidly as he flew higher in a balloon hypothesized they were
More informationDOE SBIR & STTR FY 2019 Phase 1, Release 1 Topics
Source: InternetCoast BUSINESS OPPORTUNITIES web page>>> Letter of Intent Deadline: September 4, 2018 Application Deadline: October 15, 2018 Download Solicitation Topic Details>>> 1. TECHNOLOGIES FOR MANAGING
More informationSTATUS OF ULTRA HIGH ENERGY COSMIC RAYS
STATUS OF ULTRA HIGH ENERGY COSMIC RAYS Esteban Roulet (Bariloche) COSMO / CosPA 2010, Tokyo Power law flux stochastic (Fermi) acceleration in shocks cosmic ray flux Small fractional energy gain after
More informationUltra High Energy Cosmic Rays What we have learnt from. HiRes and Auger. Andreas Zech Observatoire de Paris (Meudon) / LUTh
Ultra High Energy Cosmic Rays What we have learnt from HiRes and Auger Andreas Zech Observatoire de Paris (Meudon) / LUTh École de Chalonge, Paris, Outline The physics of Ultra-High Energy Cosmic Rays
More informationCOSMIC RAYS DAY INTRODUCTION TO COSMIC RAYS WINDWARD COMMUNITY COLLEGE - SEPTEMBER 26, 2015 VERONICA BINDI - UNIVERSITY OH HAWAII
COSMIC RAYS DAY WINDWARD COMMUNITY COLLEGE - SEPTEMBER 26, 2015 VERONICA BINDI - UNIVERSITY OH HAWAII INTRODUCTION TO COSMIC RAYS MAJOR QUESTIONS: Are there forms of matter in the Universe that do not
More informationStatus and Perspectives of the LAGO Project
Status and Perspectives of the LAGO Project 5 th Workshop on Air Shower Detection at High Altitude Paris, France Édgar F. Carrera ecarrera@usfq.edu.ec (for the LAGO Collaboration) Universidad San Francisco
More informationParticle Physics Beyond Laboratory Energies
Particle Physics Beyond Laboratory Energies Francis Halzen Wisconsin IceCube Particle Astrophysics Center Nature s accelerators have delivered the highest energy protons, photons and neutrinos closing
More informationCosmogenic neutrinos II
Cosmogenic neutrinos II Dependence of fluxes on the cosmic ray injection spectra and the cosmological evolution of the cosmic ray sources Expectations from the cosmic ray spectrum measured by the Auger
More informationImplications of recent cosmic ray results for ultrahigh energy neutrinos
Implications of recent cosmic ray results for ultrahigh energy neutrinos Subir Sarkar Neutrino 2008, Christchurch 31 May 2008 Cosmic rays have energies upto ~10 11 GeV and so must cosmic neutrinos knee
More informationAdam Tarte Holley. Postdoctoral Fellow Graduate Student Research Assistant Teaching Assistant
Adam Tarte Holley aholley@tntech.edu 1908 Brown Ave. Cookeville, TN 38501 (919) 649-0273 Department of Physics Bruner Hall 222 110 University Drive Cookeville, TN 38501 (931) 372-3145 Academic Positions
More informationHigh-energy neutrino detection with the ANTARES underwater erenkov telescope. Manuela Vecchi Supervisor: Prof. Antonio Capone
High-energy neutrino detection with the ANTARES underwater erenkov telescope Supervisor: Prof. Antonio Capone 1 Outline Neutrinos: a short introduction Multimessenger astronomy: the new frontier Neutrino
More informationThe use of ESAF software to simulate the performance of the future missions of the JEM-EUSO program
The use of software to simulate the performance of the future missions of the missions s University of Torino Torino, 11/04/2018 (UNITO) Torino, 11/04/2018 1 / 38 Overview missions s 1 2 missions 3 s 4
More informationCosmic Rays: A Way to Introduce Modern Physics Concepts. Steve Schnetzer
Cosmic Rays: A Way to Introduce Modern Physics Concepts Steve Schnetzer Rutgers CR Workshop May 19, 2007 Concepts Astrophysics Particle Physics Radiation Relativity (time dilation) Solar Physics Particle
More informationThis presentation was created based on the slides by Vitor de Souza from his talk at the 4th
This presentation was created based on the slides by Vitor de Souza http://cosmicraysschool.ufabc.edu.br/pres/vitor.odp from his talk at the 4th School on Cosmic Rays and Astrophysics UFABC - Santo André
More informationThe Physics of Ultrahigh Energy Cosmic Rays. Example Poster Presentation Physics 5110 Spring 2009 Reminder: Posters are due Wed April 29 in class.
The Physics of Ultrahigh Energy Cosmic Rays Example Poster Presentation Physics 5110 Spring 2009 Reminder: Posters are due Wed April 29 in class. 1 Introduction to Cosmic Rays References: http://www.phy.bris.ac.uk/groups/particle/pus/affo
More informationAutoreferat - Summary of professional accomplishments
Autoreferat - Summary of professional accomplishments 1. Name: Jan Pękala 2. Held diploma, scientific/academic degrees: 2007 Doctor of Philosophy degree in Physics; Institute of Nuclear Physics Polish
More informationThe Physics of Cosmic Rays
The Physics of Cosmic Rays QuarkNet summer workshop July 23-27, 2012 1 Recent History Most natural phenomena can be explained by a small number of simple rules. You can determine what these rules are by
More informationneutrino astronomy francis halzen university of wisconsin
neutrino astronomy francis halzen university of wisconsin http://icecube.wisc.edu 50,000 year old sterile ice instead of water we built a km 3 neutrino detector 3 challenges: drilling optics of ice atmospheric
More informationOVERVIEW OF THE RESULTS
VIIIth International Workshop on the Dark Side of the Universe, Buzios STUDY OF THE ULTRA HIGH ENERGY COSMIC RAYS WITH THE AUGER DATA OVERVIEW OF THE RESULTS H. Lyberis on behalf of the Pierre Auger Collaboration
More informationUltra High Energy Cosmic Rays: Observations and Analysis
Ultra High Energy Cosmic Rays: Observations and Analysis NOT A NEW PROBLEM, STILL UNSOLVED John Linsley (PRL 10 (1963) 146) reports on the detection in Vulcano Ranch of an air shower of energy above 1020
More informationTeaching Assistant Shared responsibility for labs, discussion sections, exams, homework assignments, and grades for an introductory physics class.
Patrick D. Ryan Contact Information ZEUS Wisconsin Office: +49 40-8998-2489 DESY Mobile: +49 162-106-3315 Notkestrasse 85 E-mail: pdryan@hep.wisc.edu 22607 Hamburg, Germany WWW: www.hep.wisc.edu/~pdryan
More informationSearch for isotropic microwave radiation from electron beam in the atmosphere
Search for isotropic microwave radiation from electron beam in the atmosphere a, I. S. Ohota a, Y. Inome a, D. Ikeda b, H. Sagawa b, S. Ogio c, T. Sako d, T. Shibata e, J. N. Mattherws f E-mail: tokonatu@konan-u.ac.jp
More informationThose invisible neutrinos
Those invisible neutrinos and their astroparticle physics Amol Dighe Department of Theoretical Physics Tata Institute of Fundamental Research, Mumbai Bhoutics, IITM, March 31st, 2017 Those invisible neutrinos...
More informationPoS(RPC2012)011. Results from the ARGO-YBJ experiment. Roberto Iuppa for the ARGO-YBJ collaboration
Results from the ARGO-YBJ experiment University of Rome Tor Vergata INFN Sez.ne di Roma Tor Vergata E-mail: roberto.iuppa@roma2.infn.it The ARGO-YBJ experiment consists of a 5000 m 2 single layer of Resistive
More informationSome Thoughts on Laboratory Astrophysics for UHE Cosmic Rays. Pierre Sokolsky University of Utah SABRE Workshop SLAC, March, 2006
Some Thoughts on Laboratory Astrophysics for UHE Cosmic Rays Pierre Sokolsky University of Utah SABRE Workshop SLAC, March, 2006 UHE Cosmic Ray detection (N, gamma, neutrino) Indirect - Extensive Air Shower
More informationJustin Vandenbroucke (KIPAC, Stanford / SLAC) for the Fermi LAT collaboration
Measurement of the cosmic ray positron spectrum with the Fermi LAT using the Earth s magnetic field Justin Vandenbroucke (KIPAC, Stanford / SLAC) for the Fermi LAT collaboration International Cosmic Ray
More informationCatching Neutrinos with an IceCube
Catching Neutrinos with an IceCube Mathieu Labare (for the IceCube Collaboration) Vrije Universiteit Brussel - IIHE mlabare@icecube.wisc.edu 04 04 2011, Neutrino-Gamma Workshop @ Marseille IceCube Collaboration
More informationUltra High Energy Cosmic Rays I
Ultra High Energy Cosmic Rays I John Linsley (PRL 10 (1963) 146) reports on the detection in Vulcano Ranch of an air shower of energy above 1020 ev. Problem: the microwave background radiation is discovered
More informationSiPMs in Astroparticle Physics:
SiPMs in Astroparticle Physics: KIT Activities (presently JEM-EUSO, but R&D for broader application) Advanced Technologies KIT The Research University in the Helmholtz Association www.kit.edu Standard
More informationAtmospheric Monitoring with LIDAR Systems at the Pierre Auger Cosmic Ray Observatory. Prof. Gregory Snow
Atmospheric Monitoring with LIDAR Systems at the Pierre Auger Cosmic Ray Observatory Prof. Gregory Snow NASA meeting, Omaha: 9/17/2010 2 3 The Fantastic Four 1996 Marvel Comics 4 Outline Cosmic Ray History
More informationCalibration of large water-cherenkov Detector at the Sierra Negra site of LAGO
Calibration of large water-cherenkov Detector at the Sierra Negra site of LAGO A. Galindo a, E. Moreno b, E. Carrasco a, I. Torres a, a, for the LAGO Collaboration c a Instituto Nacional de Astrofísica,
More informationUltra-High-Energy Cosmic Rays: A Tale of Two Observatories
Ultra-High-Energy Cosmic Rays: A Tale of Two Observatories RuoYu Shang Nicholas Sherer Fei Sun Bryce Thurston Measurement of the Depth of Maximumof Extensive Air Showers above 10 18 ev,"phys. Rev. Letters104(2010)
More informationTeV Future: APS White Paper
TeV Future: APS White Paper APS commissioned a white paper on the "Status and Future of very high energy gamma ray astronomy. For preliminary information, see http://cherenkov.physics.iastate.edu/wp Working
More informationAnalysis of the modulation in the first harmonic of the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
Analysis of the modulation in the first harmonic of the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory H. Lyberis 1 for the Pierre Auger Collaboration 2 1 Université
More informationIceCube: Dawn of Multi-Messenger Astronomy
IceCube: Dawn of Multi-Messenger Astronomy Introduction Detector Description Multi-Messenger look at the Cosmos Updated Diffuse Astrophysical Neutrino Data Future Plans Conclusions Ali R. Fazely, Southern
More informationFluorescence Measurements at ANL and the Auger Experiment
Fluorescence Measurements at ANL and the Auger Experiment Motivation for Fluorescence Calibrations AIRFLY Fluorescence Experiment at ANL Auger Experiment Update N 2 Molecule Vibrational Energy Levels 337nm
More informationThe Pierre Auger Project: Status and Recent Results. Pierre Auger Project. Astrophysical motivation
The Pierre Auger Project: Status and Recent Results Markus Roth Forschungszentrum Karlsruhe Markus.Roth@ik.fzk.de Astrophysical motivation Pierre Auger Project Experimental concept Status Results Summary
More informationCURRICULUM VITAE. Albrecht Karle
CURRICULUM VITAE Albrecht Karle High Energy Physics University of Wisconsin-Madison 1150 University Avenue Madison, WI 53706 USA Phone: (+1) 608-262 3945 Fax: (+1) 608-262 0800 E-mail: karle@alizarin.physics.wisc.edu
More informationRadio-detection of UHECR by the CODALEMA experiment
Radio-detection of UHECR by the CODALEMA experiment O. Ravel To cite this version: O. Ravel. Radio-detection of UHECR by the CODALEMA experiment. 30th International Cosmic Ray Conference - ICRC 07, Jul
More informationCosmic Rays and the need for heavy payloads
Cosmic Rays and the need for heavy payloads T. Gregory Guzik Department of Physics and Astronomy Louisiana State University Baton Rouge, LA LSU 04/19/07 LCANS 2007 - April 27, 2007 1 Ballooning leads the
More informationThe 7th International Workshop on Very High Energy Particle Astronomy (VHEPA2014)
The 7th International Workshop on Very High Energy Particle Astronomy (VHEPA2014) - Next Generation Explorer for Cosmic Ray Origin - T.Kifune The University of Tokyo (emeritus) Discussions for exploring/developing
More informationCosmic Ray Astronomy. Qingling Ni
Cosmic Ray Astronomy Qingling Ni What is Cosmic Ray? Mainly charged particles: protons (hydrogen nuclei)+helium nuclei+heavier nuclei What s the origin of them? What happened during their propagation?
More informationarxiv:astro-ph/ v1 28 Oct 2004
Highest Energy Cosmic Rays Angela V. Olinto arxiv:astro-ph/0410685v1 28 Oct 2004 Department of Astronomy & Astrophysics, Kavli Institute of Cosmological Physics The University of Chicago, 5640 S. Ellis
More informationarxiv: v1 [astro-ph.he] 28 Jan 2013
Measurements of the cosmic ray spectrum and average mass with IceCube Shahid Hussain arxiv:1301.6619v1 [astro-ph.he] 28 Jan 2013 Abstract Department of Physics and Astronomy, University of Delaware for
More information