LATEST RESULTS OF THE ANTARES HIGH ENERGY NEUTRINO TELESCOPE
|
|
- Jonah Bradford
- 6 years ago
- Views:
Transcription
1 Torino - 13/07/2010 LATEST RESULTS OF THE ANTARES HIGH ENERGY NEUTRINO TELESCOPE Tommaso Chiarusi INFN - Sezione Bologna on behalf of the ANTARES Collaboration
2 Physics with High Energy Cosmic νs SNR Binary systems neutrinos Microquasars Dark Matter? Exotics (magnetic monopoles, nuclearites) protons (50 Mpc) Galactic photons (10 Mpc) Extra Galactic AGN neutrons (unstables) GRB low energy particles
3 Neutrino Telescopes perform indirect measurements (Markov, 1960 ) PMTs lattice transparent media Cherenkov light charge current interaction ν μ N W μ X Upgoing μ incoming neutrino ν μ dense neutrino target track reconstruction from time and position of detected Cherenkov light assuming a θcherenkov = 43 in water
4 Sky coverage ANTARES > 75% 2 25% 75% < 25% TeV γ-sources galactic extragalactic IceCube 100% 0%
5 The ANTARES Collaboration ITEP, Moscow University of Moscow IFIC, Valencia UPV, Valencia, TUC, Barcelona NIKHEF, Amsterdam KVI Groningen NIOZ Texel CPPM, Marseille DSM/IRFU/CEA, Saclay APC Paris IPHC (IReS), Strasbourg Univ. de H.-A., Mulhouse Clermont-Ferrand IFREMER, Toulon/Brest C.O.M. Marseille LAM, Marseille University/INFN of Bari University/INFN of Bologna University/INFN of Catania University of Erlangen Reimes Sternwarte Bamberg. ISS, Bucarest GeoAzur Villefranche LNS Catania University/INFN of Pisa University/INFN of Rome University/INFN of Genova Tommaso Chiarusi PCC Torino 13/07/2010
6 The ANTARES Site Toulon La Seyne sur Mer Main cable (45km) Shore station
7 12 lines of 75 PMTs 25 storeys/line 3 PMTs/storey 885 active PMTs Instrumented volume 0.05 km 3 high PMT density so to have a good angular resolution and optimizing the effective area Tommaso Chiarusi PCC Torino 13/07/2010
8 Expected Performance (full detector) Neutrino effective area For E ν <10 PeV, A eff grows with energy due to the increase of σ ν and the muon range. For E ν >10 PeV the Earth becomes opaque to neutrinos. Angular resolution For E ν < 10 TeV, the angular resolution is dominated by the ν-μ angle. For E ν > 10 TeV, the resolution is limited by track reconstruction errors. N det =A eff Time Flux 8 A 0.3 deg angular resolution would imply a time precision better than 5 ns and OM position known to better than 2 m ANTARES actual time and spatial precisions: ~ 1.8 ns (= 1.3 ns TTS ns time calib.) on a 10 PMT and ~ 0.1 m for each OM!!
9 ANTARES deployment
10 Living under the sea: the uncorrelated single photon spurious signals Bursts in the rate from bioluminescence baseline ( 40 K + biolumin.) 40 K decays (constant) 40 khz/pmt(10, 0.5 p.e. thld) Bioluminescence (occasional) up to some MHz/PMT(10, 0.5 p.e. thld) + No beam crossing reference such as for experiments at Colliders + complex DAQ structures in extreme conditions (mandatory: minimal underwater maintaining) ALL DATA TO SHORE approach (up to 15 Gbps total)
11 Z(m) Acoustic Positioning Example for Sea current v= 25 cm/s r max = 22m Acoustic system 1 emitter (+ receiver) at each line socket 5 receivers along each line Compass and Accelerometer 1 Compass at each storey 1 Accelerometer at each storey mostly coherent movement of lines r(m) Measure every 2 min Acoustics: distance sockets - receivers Compass: Heading Accelerometer: tilt Tommaso Chiarusi PCC Torino 13/07/2010
12 Atmospheric muons and neutrinos p cosmic rays 5-line data (May-Dec 2007) line data (2008) µ νµ background 341 days detector live time 1062 neutrino candidates cosmic νµ νµ µ atmosphere Preliminary good agreement with Monte-Carlo expectation: upward-going: atmospheric neutrinos: 916 (30% syst. error) atmospheric muons: 40 (50% syst. Error) Zenith angle
13 Muon Depth Intensity Relation ANTARES data with 5 lines Tommaso Chiarusi PCC Torino 13/07/2010
14 Scrambled ANTARES Sky map of 1000 neutrinos Galactic coordinate System Earth coordinate System Tommaso Chiarusi PCC Torino 13/07/2010
15 Point source sensitivity Point source search with 5-lines data (2007) is close to be finalized. preliminary In the next weeks the ANTARES Collaboration will publish the relative upper limits Tommaso Chiarusi PCC Torino 13/07/2010
16 Dark matter searches 5-line data 2007 (68 days) 68 days detector live time Competitive with direct detection for SD cross section Flux Neutralino mass (GeV)
17 Diffuse Flux: energy estimator R = number of PMTs with prompt and late photons number of all PMTs contributing to the event muon cascade good slope for energy resolution
18 Diffuse Flux: unblindig the data events/bin 10 2 E test -7-2 = 10 GeV cm s -1 sr -1 Atms, no R cut Atms, R 1.31 Signal, no R cut Signal, R νprompt (Bartol+RQPM) % log 10 (E /GeV) R = number of PMTs with prompt and late photons number of all PMTs contributing to the event Tommaso Chiarusi PCC Torino 13/07/2010
19 Diffuse Flux: upper limit with data preliminary MACRO: Astropart.Phys. 19:1-13,2003. BAIKAL, Astronomy Letters, 2009, Vol. 35, No. 10, pp AMANDA-II (807 d) Phys.Rev.D76:042008,2007 IceCube: Astrop. Phys. 20 (2004) 507 WB= Waxman & Bahcall, PRD59 (1999) MPR98, PRD 63 (2001) SDSS91: Phys. Rev. Lett. 66(91)2697 Tommaso Chiarusi PCC Torino 13/07/2010
20 Ongoing combined searches Receive GRB alerts from Satellites (Fermi, Swift...) search for coincident neutrinos within time window (~100 seconds) Send neutrino cluster alert for optical follow-up Trigger: multiple / HE single neutrino event; Reconstruction on-line (<10ms) Alert message to Tarot Telescope in La Silla (Chile) Tarot takes 6 images of 3 minutes immediately and after 1, 3, 9 and 27 days sending alerts to the ROTSE system (4 telescopes) since 3 months Correlation with AUGER source distribution investigate directional correlation of neutrinos and UHE particles Correlation with VIRGO-LIGO signals investigate correlation of neutrinos and gravitational waves Tommaso Chiarusi PCC Torino 13/07/2010
21 Conclsions ANTARES is continuously taking data has a broad physics program determined the most sensitive upper limit on diffuse flux complements the sky coverage of IceCube paves the way for KM3NeT Tommaso Chiarusi PCC Torino 13/07/2010
22 THANK YOU! Essential Bibliography 1. T. Chiarusi and M. Spurio, 2010, High-Energy Astrophysics with Neutrino Telescope, European Physics Journal C 65, nn. 3-4, J. A. Aguilar et al. Transmission of light in deep sea water at the site of the Antares neutrino telescope. Astropart. Phys. 23 (2005) P. Amram et al. Sedimentation and Fouling of Optical Surfaces at the ANTARES Site. Astropart Phys. 19 (2003) P. Amram et al. The ANTARES optical module. Nucl. Instr. Meth. A484 (2002) M. Ageron et al. Studies of a full scale mechanical prototype line for the ANTARES neutrino telescope and tests of a prototype instrument for deep-sea acoustic measurements. Nucl. Instrum. Meth. A581 (2007) J. A. Aguilar, The Data Acquisition System of the ANTARES neutrino telescope, Nucl. Instrum. Meth. A 570 (2007) A.Margiotta(ANTARESColl.), Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-line ANTARES detector. Nucl. Instrum. Meth. A602 (2009) 76. arxiv: [astro-ph]. 8. G. Carminati, A. Margiotta, M. Spurio. MUons from Parametric formulas: A fast Generator of atmospheric μ-bundles for neutrino telescopes (MUPAGE). Nucl. Instr. Methods A602 (2009) J.A. Aguilar et al, Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector, in press on Astropart. Physics (ASTROPARTPHYS-D R2)
23 SPARE SLIDES
24 Observation of induced electromagnetic showers from muon tracks The light from EM shower is produced in one point on the muon path and it arrives delayed at PMT preliminary
25 ANGULAR RESOLUTION angular resolution = difference between reconstructed and MC generated angles vs. neutrino energy µ rec µ gener. dominated by kinema)cs ν µ rec ν gener. µ dominated by reconstruc)on angular resolu+on < 0.2 above 10 TeV limited tracking accuracy due to <me resolu<on: Light scaaering σ ~ 1.0 ns TTS in PMT σ ~ 1.3 ns <me calibra<on σ < 0.5 ns OM posi<on σ < 10 cm 25 ( σ < 0.5 ns)
26 THE ANTARES DETECTOR POSITIONING SYSTEM REAL TIME POSITIONING Acous<c posi<oning system + set of <ltmeters and compasses. Transceivers (RxTx) on the boaom of the lines, 4 autonomous transponders around the apparatus. 5 hydrophones (Rx) per line at specific heights. Tiltmeter and compass per storey, sound velocimeters (various depths). RECONSTRUCTION OF THE LINE SHAPE GLOBAL χ 2 FIT TO LINE SHAPE MODEL (BEHAVIOUR OF LINE: SEA CURRENT) Hydrophone posi)on rela)ve to line base loca)on (20 days) hydrophone Acoustic transceiver Acoustic transceiver Resolu)on be2er than 10 cm
27 TIME CALIBRATION Time difference between the LED OB and an OM 3 OMs σ = 0.4 ns 27 Op+cal LED beacon - Electronics + calibra)on σ ~ 0.5 ns - TTS in photomul)pliers σ ~ 1.3 ns - Light sca2ering + dispersion in sea water σ ~ 1.5 ns at 40 m Angular resolu+on 0.3 o (for E ν > 10 TeV ) Including the acous)c posi)on resolu)on and the ν- µ angle
28 ATTENUATION LENGTH MEASUREMENTS R min R max 28 The biggest challenge is to determine the separate contribu4on of absorp'on and sca*ering
29 IN SITU CALIBRATION WITH 40 K Integral under peak = rate of correlated coincidences γ Gaussian peak on coincidence plot Cherenkov γ e - (β decay) 40 K Peak offset 40 Ca 29 No dependence on bioluminescent ac<vity has been observed Cross check of <me calibra<on High precision (~5%) monitoring of OM efficiencies
30 Physics with High Energy Cosmic νs Understanding production mechanism ( cosmic accelerators ) of HE cosmic rays SNR Study very energetic objects: galactic: SN remnants, microquasars.. extragalactic: GRB, AGN, ; Search for Dark matter (wimps) Binary systems Exotic (magnetic monopoles, nuclearites) Microquasars Dark Matter? Exotics (magnetic monopoles, nuclearites) AGN GRB
31 Latest results of the ANTARES high-energy neutrino telescope The ANTARES high-energy neutrino telescope, fully functional since May 2008, is based on the detection of Cherenkov light produced in sea water by neutrinoinduced muons as well as electromagnetic or hadronic showers. It consists of a three-dimensional array of 885 photomultipliers distributed over 12 lines and installed at a depth of 2500 m in the Mediterranean Sea, 40 km off the French coast. The main goal of the experiment is the search for highenergy neutrinos from astrophysical sources such as AGNs, GRBs and SGRs or possibly from WIMP annihilation in the Sun or in the Galactic Halo. The telescope is sensitive to neutrinos with energy greater than few hundred GeV, with an effective area for upward muon detection which reaches 0.05 km2 at the highest energies. In this talk we review the current status of the detector; we give an overview on the atmospheric muon and neutrino analyses and present the first searches for point-like neutrino sources and diffuse flux of VHE neutrinos using data from Dec to Dec Abstract only for review this slide will be cut
High energy neutrino astronomy with the ANTARES Cherenkov telescope
High energy neutrino astronomy with the ANTARES Cherenkov telescope P.Vernin CEA/Irfu/SPP On behalf of the ANTARES collaboration IWARA 2009 Conference Maresias, Sao Paulo, Brazil, 4-8/10/2009 i r f u saclay
More informationResent results from Antares Aart Heijboer, Nikhef on behalf of the Antares collaboration.
Resent results from Antares Aart Heijboer, Nikhef on behalf of the Antares collaboration. 1 Neutrino Astronomy Protons/ Cosmic Rays (CR): Detected on Earth up to extremely high energies: 108 TeV Hard to
More informationTHE ANTARES NEUTRINO TELESCOPE: CURRENT STATUS AND FIRST RESULTS
THE ANTARES NEUTRINO TELESCOPE: CURRENT STATUS AND FIRST RESULTS 12th Topical Seminar on Innovative Particle and Radiation Detectors ( 07 10 June 2010 Siena, Italy Harold Yepes-Ramírez IFIC (CSIC-UV),
More informationJ. P. Gómez-GonzálezGonzález
STATUS OF THE ANTARES NEUTRINO TELESCOPE 5th Iberian cosmology meeting 29-31 March 2010 Oporto J. P. Gómez-GonzálezGonzález Outline Physicswithneutrino telescopes Detectionprincipleand detector description
More informationStatus and first results of the ANTARES neutrino telescope
Status and first results of the ANTARES neutrino telescope research goals the detector setup status and performance first results summary Heide Costantini INFN, Genova, Italy The Cosmic Ray (CR) Spectrum
More informationMeasurement of the atmospheric νμ energy spectrum and improved limits on the νμ diffuse fluxes with ANTARES
Rencontres de Moriond La Thuile, 9-16 March 2013 Measurement of the atmospheric νμ energy spectrum and improved limits on the νμ diffuse fluxes with ANTARES Simone Biagi University of Bologna & INFN on
More informationResults from the ANTARES Deep Sea Neutrino Telescope
M.Spurio-MG13 @ Stockholm Results from the ANTARES Deep Sea Neutrino Telescope Maurizio Spurio On behalf of the ANTARES Collaboration Università di Bologna and INFN Science with Deep Sea Neutrino Telescopes
More informationHigh Energy Astrophysics with underwater neutrino detectors. Marco Anghinolfi INFN, Genova, Italia
High Energy Astrophysics with underwater neutrino detectors Marco Anghinolfi INFN, Genova, Italia Outline of the talk Neutrino astronomy The potential sources The ANTARES detector and the first physics
More informationThe ANTARES Telescope Status and Results
DBD 2011 Osaka, November 14-17 The ANTARES Telescope Status and Results Simone Biagi Department of physics and INFN Bologna, Italy Recent Papers Point Sources: ApJL accepted arxiv:1108.0292 [astro-ph.he]
More informationLawrence Berkeley National Laboratory Lawrence Berkeley National Laboratory
Lawrence Berkeley National Laboratory Lawrence Berkeley National Laboratory Title Neutrino Physics with the IceCube Detector Permalink https://escholarship.org/uc/item/6rq7897p Authors Kiryluk, Joanna
More informationSearch for a diffuse cosmic neutrino flux with ANTARES using track and cascade events
Search for a diffuse cosmic neutrino flux with ANTARES using track and cascade events Jutta Schnabel on behalf of the ANTARES collaboration Erlangen Centre for Astroparticle Physics, Erwin-Rommel Str.
More informationRecent Results from the ANTARES experiment
Recent Results from the ANTARES experiment Manuela Vecchi on behalf of the ANTARES Collaboration University of Roma La Sapienza and INFN ICATPP09- Como: October 6th 2009 Outline -astronomy: what, where,
More informationMediterranean Neutrino Telescopes
Mediterranean Neutrino Telescopes New Views of the Universe Chicago, December 2005 Juande D. Zornoza (IFIC UW-Madison) Advantages: Neutrino Astronomy Neutrino Astronomy is a quite recent and very promising
More informationLake Baikal: from Megaton to Gigaton. Bair Shaybonov, JINR, Dubna on behalf of the Baikal Collaboration
Lake Baikal: from Megaton to Gigaton Bair Shaybonov, JINR, Dubna on behalf of the Baikal Collaboration TAUP09, Rome, July 2009 Outline Status of the Baikal Detector Selected Results obtained from NT200
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 informationHigh Energy Neutrino Astronomy
High Energy Neutrino Astronomy VII International Pontecorvo School Prague, August 2017 Christian Spiering, DESY Zeuthen Content Lecture 1 Scientific context Operation principles The detectors Atmospheric
More informationDetection of transient sources with the ANTARES telescope. Manuela Vecchi CPPM
Detection of transient sources with the ANTARES telescope Manuela Vecchi CPPM Multimessenger Astronomy CRs astronomy feasible at energies higher than 1019 ev extragalactic origin UHECRs horizon limited
More informationHigh Energy Neutrino Astrophysics Latest results and future prospects
High Energy Neutrino Astrophysics Latest results and future prospects C. Spiering, Moscow, August 22, 2013 DETECTION PRINCIPLE Detection Modes Muon track from CC muon neutrino interactions Angular resolution
More informationResults from the ANTARES neutrino telescope with six years of data
Available online at www.sciencedirect.com ScienceDirect Physics Procedia 61 (2015 ) 450 458 Results from the ANTARES neutrino telescope with six years of data M. Spurio, on the behalf of the ANTARES Collaboration
More informationNeutrino Mass Hierarchy and other physics in H 2 0 (ORCA & PINGU) Aart Heijboer Nikhef, Amsterdam, KM3NeT collaboration
1 Neutrino Mass Hierarchy and other physics in H 2 0 (ORCA & PINGU) Aart Heijboer Nikhef, Amsterdam, KM3NeT collaboration sign unknown (vacuum) sign known 2 Mass Hierarchy matter Hierarchy important for
More informationSearch for diffuse cosmic neutrino fluxes with the ANTARES detector
Search for diffuse cosmic neutrino fluxes with the ANTARES detector Vladimir Kulikovskiy The ANTARES Collaboration 1 Overview ANTARES description Full sky searches Special region searches Fermi bubbles
More informationSEARCH FOR NUCLEARITES WITH THE ANTARES DETECTOR *
Romanian Reports in Physics, Vol. 64, No. 1, P. 325 333, 2012 SEARCH FOR NUCLEARITES WITH THE ANTARES DETECTOR * GABRIELA EMILIA PĂVĂLAŞ Institute for Space Science, Atomistilor 409, PO Box Mg-23, Magurele,
More informationFirst results from the NEMO Phase 1 experiment
First results from the NEMO Phase 1 experiment Isabella Amore a,b for the NEMO Collaboration a Dipartimento di Fisica e Astronomia, Università di Catania, Italy b INFN Laboratori Nazionali del Sud, Catania,
More informationSearch for high energy neutrino astrophysical sources with the ANTARES Cherenkov telescope
Dottorato di Ricerca in Fisica - XXVIII ciclo Search for high energy neutrino astrophysical sources with the ANTARES Cherenkov telescope Chiara Perrina Supervisor: Prof. Antonio Capone 25 th February 2014
More informationNeutrino Astronomy. Ph 135 Scott Wilbur
Neutrino Astronomy Ph 135 Scott Wilbur Why do Astronomy with Neutrinos? Stars, active galactic nuclei, etc. are opaque to photons High energy photons are absorbed by the CMB beyond ~100 Mpc 10 20 ev protons,
More informationTHE KM3NET NEUTRINO TELESCOPE IN THE MEDITERRANEAN SEA
THE KM3NET NEUTRINO TELESCOPE IN THE MEDITERRANEAN SEA PIERA SAPIENZA ON BEHALF OF THE KM3NET COLLABORATION FRONTIERS OF RESEARCH ON COSMIC RAY GAMMA - LA PALMA 26-29 AUGUST 2015 OUTLINE MOTIVATION DETECTOR
More informationKM3NeT. P. Piattelli, INFN SciNeGHE 2010, Trieste, september
KM3NeT, INFN SciNeGHE 2010, Trieste, september 8 10 2010 Overview Introduction The KM3NeT Technical Design Report KM3NeT physics performances New developments Summary 2 Motivations for High Energy neutrino
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 informationSearch for Astrophysical Neutrino Point Sources at Super-Kamiokande
Search for Astrophysical Neutrino Point Sources at Super-Kamiokande Yusuke Koshio for Super-K collaboration Kamioka, ICRR, Univ. of Tokyo LNGS, INFN Super-Kamiokande detector Recent results of search for
More informationSELECTED RESULTS OF THE ANTARES TELESCOPE AND PERSPECTIVES FOR KM3NET. D. Dornic (CPPM) on behalf the ANTARES Coll.
SELECTED RESULTS OF THE ANTARES TELESCOPE AND PERSPECTIVES FOR KM3NET D. Dornic (CPPM) on behalf the ANTARES Coll. MORIOND VHEPU @ La Thuile, March 2017 Neutrino telescopes: science scope Low$Energy$$
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 informationA M A N DA Antarctic Muon And Neutrino Detector Array Status and Results
A M A N DA Antarctic Muon And Neutrino Detector Array Status and Results (http://www.amanda.uci.edu) Peter Steffen DESY Zeuthen, Germany TAUP 2003 The AMANDA Collaboration ª 150 members New Zealand Japan
More informationSearch for Point-like. Neutrino Telescope
Search for Point-like Sources with the ANTARES Neutrino Telescope Francisco Salesa Greus IFIC (CSIC Universitat de València, Spain) On behalf of the ANTARES collaboration Outline Neutrino astronomy. The
More informationFirst results of the ANTARES neutrino telescope
Journal of Physics: Conference Series First results of the ANTARES neutrino telescope To cite this article: C Bigongiari and the Antares Collaboration 2009 J. Phys.: Conf. Ser. 173 012024 Related content
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 informationKM3NeT and Baikal-GVD New Northern Neutrino Telescopes
KM3NeT and Baikal-GVD New Northern Neutrino Telescopes E. de Wolf Nikhef/University of Amsterdam VHEPU, 3-9 August 2014 ICISE, Quy Nhon, Vietnam KM3NeT and GVD New Northern Neutrino Telescopes Gigaton
More informationSURFACE ARRAY Détecteur de surface pour ANTARES JP Ernenwein CPPM
SURFACE ARRAY Détecteur de surface pour ANTARES JP Ernenwein CPPM GDR 29/10/2009 ANTARES OM 14.5 m 10 PMT 350 m 25 étages ANTARES, 2475m, 3 PMT/floor 12 lines of 25 floors 885 PMTs 100 m 70 m floor JUNCTION
More informationRecent Results from ANTARES and prospects for KM3NeT. Aart Heijboer. Nikhef, Amsterdam On behalf of the ANTARES and KM3NeT collaborations
Recent Results from ANTARES and prospects for KM3NeT Aart Heijboer Nikhef, Amsterdam On behalf of the ANTARES and KM3NeT collaborations European Neutrino Telescopes 2 * and ANTARES ANTARES KM3NeT * * Münster
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 informationProgress and latest results from Baikal, Nestor, NEMO and KM3NeT
Progress and latest results from Baikal, Nestor, NEMO and KM3NeT Emilio Migneco Dipartimento di Fisica e Astronomia Università di Catania, Via S.Sofia 64, 95123, Catania, Italy INFN Laboratori Nazionali
More informationStatus of the BAIKAL-GVD Project
Status of the BAIKAL-GVD Project Zh.-A. Dzhilkibaev (INR, Moscow) for the Baikal Collaboration Rome, May 26, 2011 ANTARES KM3NeT (~2017) A N N NT200+/Baikal-GVD (~2018) In opera)on IceCube (2011) Shore
More informationMulti-Messenger Programs in ANTARES: Status and Prospects. Véronique Van Elewyck Laboratoire AstroParticule et Cosmologie (Paris)
Multi-Messenger Programs in ANTARES: Status and Prospects Laboratoire AstroParticule et Cosmologie (Paris) An overview Externally triggered neutrino searches: the example of GRBs Strategies for data acquisition
More informationFollow-up of high energy neutrinos detected by the ANTARES telescope
Follow-up of high energy neutrinos detected by the ANTARES telescope, on behalf of the ANTARES, TAROT, ROTSE, MASTER and SWIFT Collaborations Aix Marseille Université, CNRS/IN2P3, CPPM UMR 7346, 13288,
More informationNeutrino & γ-ray astronomy
Neutrino & γ-ray astronomy Looking for signals directly from cosmic-ray sources Q: why is this needed? Berlin, 2 Oct 2009 Tom Gaisser 1 Werner Hofmann, TeV PA 2009 R. Chaves ICRC 2009 The Galactic Plane
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 informationStudy of the high energy Cosmic Rays large scale anisotropies with the ANTARES neutrino telescope
Journal of Physics: Conference Series PAPER OPEN ACCESS Study of the high energy Cosmic Rays large scale anisotropies with the ANTARES neutrino telescope To cite this article: Giulia Illuminati 2016 J.
More informationResults from the ANTARES neutrino telescope
EPJ Web of Conferences 116, 11006 (2016) DOI: 10.1051/epjconf/201611611006 C Owned by the authors, published by EDP Sciences, 2016 Results from the ANTARES neutrino telescope M. Spurio, on behalf of the
More informationAstroparticle Physics with IceCube
Astroparticle Physics with IceCube Nick van Eijndhoven nickve.nl@gmail.com http://w3.iihe.ac.be f or the IceCube collaboration Vrije Universiteit Brussel - IIHE(ULB-VUB) Pleinlaan 2, B-1050 Brussel, Belgium
More informationSearches for Dark Matter Annihilations in the Sun and Earth with IceCube and DeepCore. Matthias Danninger for the IceCube collaboration
Searches for Dark Matter Annihilations in the Sun and Earth with IceCube and DeepCore for the IceCube collaboration Content Overview: IceCube (see IceCube status plenary talk by D. Williams ) DeepCore
More informationNeutrino Astronomy with AMANDA
Neutrino Astronomy with AMANDA NeSS 2002 Washington, D.C. Sep 20, 2002 Albrecht Karle University of Wisconsin-Madison karle@alizarin.physics.wisc.edu The AMANDA Collaboration 7 US, 9 European and 1 South
More informationPoS(EPS-HEP2017)008. Status of the KM3NeT/ARCA telescope
for the KM3NeT Collaboration Laboratori Nazionali del Sud, INFN, Catania, Italy E-mail: distefano_c@lns.infn.it The KM3NeT Collaboration has started the implementation of the ARCA detector, the next generation
More informationThe ANTARES neutrino telescope:
The ANTARES neutrino telescope: main results and perspectives for KM3NeT Sergio Navas University of Granada, Spain On behalf of the ANTARES and KM3NeT Collaborations 14th Rencontres du Vietnam: Very High
More informationKurt Woschnagg UC Berkeley
Neutrino Astronomy at the South Pole Latest results from IceCube Kurt Woschnagg UC Berkeley SLAC Summer Institute August 3, 2011 Neutrinos as Cosmic Messengers Neutrinos and the Origin of Cosmic Rays Cosmic
More informationKM3NeT-ARCA project status and plan
EPJ Web of Conferences 116, 11003 (2016) DOI: 10.1051/epjconf/201611611003 C Owned by the authors, published by EDP Sciences, 2016 KM3NeT-ARCA project status and plan R. Coniglione a on behalf of the KM3NeT
More informationLa rivelazione di neutrini astrofisici
La rivelazione di neutrini astrofisici T. Montaruli Università di Bari & INFN Neutrino Astrophysics Motivations Physics Issues Current Neutrino Telescopes and Experimental Results Future Outlook XV IFAE,
More informationParticle Physics with Neutrino Telescope Aart Heijboer, Nikhef
Particle Physics with Neutrino Telescope Aart Heijboer, Nikhef 1 high energy Quanta from the Universe (why look for neutrinos) Universe contains very high Energy particle accelerators (E = up to 10 6
More informationUnderwater Neutrino Telescopes
Neutrino Oscillation Workshop 2008 (NOW 2008) Conca Specchiulla / Otranto, Italy, 6-13 Sept. 2008 Underwater Neutrino Telescopes Uli Katz ECAP / Univ. Erlangen 11.09.2008 Introduction A few words on physics
More informationGamma-rays, neutrinos and AGILE. Fabrizio Lucarelli (ASI-SSDC & INAF-OAR)
Gamma-rays, neutrinos and AGILE Fabrizio Lucarelli (ASI-SSDC & INAF-OAR) Outlook 2 Overview of neutrino astronomy Main IceCube results Cosmic neutrino source candidates AGILE search for γ-ray counterparts
More informationin multimessenger astrophysics.
High Energy Neutrino detection in multimessenger astrophysics. Antonio Capone, University "La Sapienza" and I.N.F.N. Roma, Italy at the The Future of Research on Cosmic Gamma Rays La Palma, Canary Islands
More informationStatus and Perspectives for KM3NeT/ORCA
, on behalf of the KMNeT Collaboration Centre de Physique des Particules de Marseille, France E-mail: quinn@cppm.inp.fr The KMNeT Collaboration is constructing neutrino detectors at depths of 7 m and m
More informationRecent results of the ANTARES neutrino telescope
Recent results of the ANTARES neutrino telescope Juan José Hernández-Rey, and (for the ANTARES Collab.) Citation: AIP Conference Proceedings 1666, 040002 (2015); doi:.63/1.4915551 View online: https://doi.org/.63/1.4915551
More informationNeutrinos from the Milky Way. 18th Symposium on Astroparticle Physics in the Netherlands Erwin Visser
Neutrinos from the Milky Way 18th Symposium on Astroparticle Physics in the Netherlands 23-10-2013 Erwin Visser Outline How are these neutrinos produced? Why look for them? How to look for them The ANTARES
More informationPHY326/426 Dark Matter and the Universe. Dr. Vitaly Kudryavtsev F9b, Tel.:
PHY326/426 Dark Matter and the Universe Dr. Vitaly Kudryavtsev F9b, Tel.: 0114 2224531 v.kudryavtsev@sheffield.ac.uk Indirect searches for dark matter WIMPs Dr. Vitaly Kudryavtsev Dark Matter and the Universe
More informationSearch for high-energy neutrinos from GRB130427A with the ANTARES neutrino telescope
Journal of Physics: Conference Series PAPER OPEN ACCESS Search for high-energy neutrinos from GRB130427A with the ANTARES neutrino telescope To cite this article: Silvia Celli 2016 J. Phys.: Conf. Ser.
More informationPERSPECTIVES of HIGH ENERGY NEUTRINO ASTRONOMY. Paolo Lipari Vulcano 27 may 2006
PERSPECTIVES of HIGH ENERGY NEUTRINO ASTRONOMY Paolo Lipari Vulcano 27 may 2006 High Energy Neutrino Astrophysics will CERTAINLY become an essential field in a New Multi-Messenger Astrophysics What is
More informationNEUTRINO ASTRONOMY AT THE SOUTH POLE
NEUTRINO ASTRONOMY AT THE SOUTH POLE D.J. BOERSMA The IceCube Project, 222 West Washington Avenue, Madison, Wisconsin, USA E-mail: boersma@icecube.wisc.edu A brief overview of AMANDA and IceCube is presented,
More informationTowards Neutrino Astronomy with IceCube+ANTARES+KM3NeT
Towards Neutrino Astronomy with IceCube+ANTARES+KM3NeT Vincent Bertin (CPPM) on behalf of Damien Dornic (CPPM) FCPPL meeting @ Marseille Marseille 25 May 2018 NEUTRINO AS COSMIC MESSENGER Neutrinos: smoking
More informationAntonio Capone Univ. La Sapienza INFN - Roma
Observations of HE Neutrino and Multimessenger AstroParticle Physics Antonio Capone Univ. La Sapienza INFN - Roma 1 Talk outline High Energy Astrophysical Neutrino Detection in a multi-messenger scenario
More informationneutrino astronomy francis halzen University of Wisconsin
neutrino astronomy francis halzen University of Wisconsin http://icecube.wisc.edu menu neutrino astronomy cosmic ray accelerators and neutrinos: km 3 neutrino detectors Amanda and Antares: first generation
More informationA Search for Point Sources of High Energy Neutrinos with AMANDA-B10
A Search for Point Sources of High Energy Neutrinos with AMANDA-B10 Scott Young, for the AMANDA collaboration UC-Irvine PhD Thesis: http://area51.berkeley.edu/manuscripts Goals! Perform an all-sky search
More informationarxiv:astro-ph/ v1 7 Oct 1999
Search for high energy neutrinos with the BAIKAL underwater detector NT-96 arxiv:astro-ph/9910133v1 7 Oct 1999 V.A.Balkanov a,i.a.belolaptikov g, L.B.Bezrukov a, N.M.Budnev b, A.G.Chensky b, I.A.Danilchenko
More informationHigh Energy Neutrino Astrophysics with IceCube
High Energy Neutrino Astrophysics with IceCube Konstancja Satalecka, DESY Zeuthen UCM, 25th February 2011 OUTLINE Neutrino properties Cosmic Neutrinos Neutrino detection Ice/Water Cerenkov Detectors Neutrino
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 informationKM3NeT. Astro-particle and Oscillations Research with Cosmics in the Abyss (ARCA & ORCA)
KM3NeT Astro-particle and Oscillations Research with Cosmics in the Abyss (ARCA & ORCA) International Solvay Institutes 27 29 May 2015, Brussels, Belgium. Maarten de Jong 1 Introduction KM3NeT is a new
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 information(7) Instrumentation in high energy neutrino experiments
(7) Instrumentation in high energy neutrino experiments Scientific Objectives Solar Neutrinos & Atmospheric Neutrinos High Energy Neutrino Detection in Ice (AMANDA & ICECUBE) High Energy Neutrino Detection
More informationNeutrino Oscillations and Astroparticle Physics (5) John Carr Centre de Physique des Particules de Marseille (IN2P3/CNRS) Pisa, 10 May 2002
Neutrino Oscillations and Astroparticle Physics (5) John Carr Centre de Physique des Particules de Marseille (IN2P3/CNRS) Pisa, 10 May 2002 n High Energy Astronomy Multi-Messanger Astronomy Cosmic Rays
More informationIceCube & DeepCore Overview and Dark Matter Searches. Matthias Danninger for the IceCube collaboration
IceCube & DeepCore Overview and Dark Matter Searches for the IceCube collaboration Content Overview: IceCube DeepCore (DOMs, geometry, deep ice properties, trigger & filter) Dark Matter searches: (current
More informationExperimental high energy neutrino astronomy
Mem. S.A.It. Suppl. Vol. 9, 363 c SAIt 2006 Memorie della Supplementi Experimental high energy neutrino astronomy E. Migneco 1,2 1 Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Sud, Via
More informationPublications 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 informationA new IceCube starting track event selection and realtime event stream
A new IceCube starting track event selection and realtime event stream Sarah Mancina Kyle Jero Advisor: Albrecht Karle Neutrino Parallel TeVPA 2017 Columbus, OH August 8th, 2017 IceCube and Atmospheric
More informationMeasuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2)
Measuring the neutrino mass hierarchy with atmospheric neutrinos in IceCube(-Gen2) Beyond the Standard Model with Neutrinos and Nuclear Physics Solvay Workshop November 30, 2017 Darren R Grant The atmospheric
More informationIceCube: Ultra-high Energy Neutrinos
IceCube: Ultra-high Energy Neutrinos Aya Ishihara JSPS Research Fellow at Chiba University for the IceCube collaboration Neutrino2012 at Kyoto June 8 th 2012 1 Ultra-high Energy Neutrinos: PeV and above
More informationPoS(NOW2016)041. IceCube and High Energy Neutrinos. J. Kiryluk (for the IceCube Collaboration)
IceCube and High Energy Neutrinos Stony Brook University, Stony Brook, NY 11794-3800, USA E-mail: Joanna.Kiryluk@stonybrook.edu IceCube is a 1km 3 neutrino telescope that was designed to discover astrophysical
More informationNeutrino Astronomy at the South Pole AMANDA and IceCube
1 Neutrino Astronomy at the South Pole AMANDA and IceCube Ignacio Taboada University of California - Berkeley Topics in Astroparticle and Underground Physics Zaragoza. Sept 10-14, 2005 2 The IceCube Collaboration
More informationAPP-VII Introduction to Astro-Particle Physics. Maarten de Jong
APP-VII Introduction to Astro-Particle Physics Maarten de Jong 1 High-energy neutrino astronomy How to build a km 3 detector in the sea 1960 Markov s idea: Use sea water as target/detector ν µ + N µ +
More informationA Summary of recent Updates in the Search for Cosmic Ray Sources using the IceCube Detector
A Summary of recent Updates in the Search for Cosmic Ray Sources using the IceCube Detector The IceCube Collaboration E-mail: tessa.carver@unige.ch In 2012 the IceCube detector observed the first clear
More informationMulti-wavelength follow-up observations of ANTARES neutrino alerts
Multi-wavelength follow-up observations of ANTARES neutrino alerts D. Dornic (CPPM) D. Turpin (IRAP), M. Ageron, V. Bertin, J. Brunner, A. Mathieu (CPPM), F. Schüssler, B. Vallage (CEA/IRFU), S. Basa (LAM)
More informationIndirect detection of Dark Matter with the ANTARES Neutrino Telescope
EPJ Web of Conferences 116, 04002 (2016) DOI: 10.1051/epjconf/201611604002 C Owned by the authors, published by EDP Sciences, 2016 Indirect detection of Dark Matter with the ANTARES Neutrino Telescope
More informationIndirect Dark Matter Detection
Indirect Dark Matter Detection Martin Stüer 11.06.2010 Contents 1. Theoretical Considerations 2. PAMELA 3. Fermi Large Area Telescope 4. IceCube 5. Summary Indirect Dark Matter Detection 1 1. Theoretical
More informationVERS UNE ASTRONOMIE NEUTRINO AVEC IceCube+ANTARES+KM3NeT
VERS UNE ASTRONOMIE NEUTRINO AVEC IceCube+ANTARES+KM3NeT DAMIEN DORNIC (CPPM) CFR Cos: Meeting de la communauté de recherche sur le rayonnement cosmique!! APC - 26-28 mars 2018 NEUTRINO AS COSMIC MESSENGER
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 informationThe KM3NeT Project: A km 3 Scale Mediterranean Neutrino Telescope and Deep-Sea Research Infrastructure
ESFRI, Astronomy & Astroparticles Panel Brussels, November 24, 2005 The KM3NeT Project: A km 3 Scale Mediterranean Neutrino Telescope and Deep-Sea Research Infrastructure Uli Katz Univ. Erlangen on behalf
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 informationMultiwavelength Search for Transient Neutrino Sources with IceCube's Follow-up Program
Multiwavelength Search for Transient Neutrino Sources with IceCube's Follow-up Program Nora Linn Strotjohann for the DESY Real-Time Group GROWTH Meeting at Caltech, July 26th 2016 The IceCube Neutrino
More informationIceCube Results & PINGU Perspectives
1 IceCube Results & PINGU Perspectives D. Jason Koskinen for the IceCube-PINGU Collaboration koskinen@nbi.ku.dk September 2014 Neutrino Oscillation Workshop Otranto, Lecce, Italy 2 IceCube Detector ~1km
More informationSearches for astrophysical sources of neutrinos using cascade events in IceCube
Searches for astrophysical sources of neutrinos using cascade events in IceCube Mike Richman TeVPA 2017 August 8, 2017 Source Searches with IceCube Cascades TeVPA 17 Mike Richman (Drexel University) 1
More informationEeV Neutrinos in UHECR Surface Detector Arrays:
EeV Neutrinos in UHECR Surface Detector Arrays: OBSERVATORY Challenges & Opportunities Karl-Heinz Kampert Bergische Universität Wuppertal High-Energy neutrino and cosmic ray astrophysics - The way forward
More informationSEARCHES OF VERY HIGH ENERGY NEUTRINOS. Esteban Roulet CONICET, Centro Atómico Bariloche
SEARCHES OF VERY HIGH ENERGY NEUTRINOS Esteban Roulet CONICET, Centro Atómico Bariloche THE NEUTRINO SKY THE ENERGETIC UNIVERSE multimessenger astronomy γ ν p γ rays (Fermi) ν (Amanda) UHE Cosmic rays
More informationOrigin of Cosmic Rays
Origin of Cosmic Rays Part 2: Neutrinos as Cosmic Ray messengers Lecture at the J. Stefan Institute Ljubljana within the course: 'Advanced particle detectors and data analysis' Hermann Kolanoski Humboldt-Universität
More information