Results from the ANTARES Deep Sea Neutrino Telescope
|
|
- Avice Bryant
- 6 years ago
- Views:
Transcription
1 Stockholm Results from the ANTARES Deep Sea Neutrino Telescope Maurizio Spurio On behalf of the ANTARES Collaboration Università di Bologna and INFN
2 Science with Deep Sea Neutrino Telescopes High energy neutrino astrophysics: galactic: SN, SNRs, m-quasars, molecular clouds, etc extra-galactic: AGNs, GRBs, choked-grbs, GZK, etc... Search for New Physics: Dark matter (Sun, Galatic Centre), Monopoles, nuclearites,?? Earth-Sea Science: oceanography, sea biology, seismology, environmental monitoring... SNR oscillations dark matter m-quasars GRBs magnetic Fermi-bubbles monopole GeV-100 GeV GeV-TeV TeV-PeV PeV-EeV > EeV 2
3 Stockholm 3 Neutrinos and Multi-Messenger Astronomy Protons/ Cosmic Rays: Detected on Earth up to extremely high energies: 10 8 TeV Hard to study sources due to deflection by magnetic fields Photons: Produced in leptonic (synchrotron, IC) and hadronic ( 0 ) processes Absorbed at higher energies and large distances Neutrinos (and GW): Unambiguous signature of hadronic acceleration Not deflected by magnetic fields or absorbed by dust Horizon not limited by interaction with CMB/IR Can escape from region of high matter density Can be time correlated with optical signals hadronic accelerators exist, but where? leptonic vs hadronic models identify Galactic and extragalactic cosmic ray sources
4 Stockholm Cosmic Rays, photons and neutrinos Hadronic cascades (as for atmospheric showers) p/a + p/ m m e e m m m e e m e : m : =1:2:0 source oscillatio ns e : m : =1:1:1 Earth Primary acceleration («Bottom-Up») Stochastics shocks (Fermi mechanism) Explosion /Accretion / Core collapse Benchmark Extra Gal. flux Waxman-Bahcall ~ 500 events /yr/ km 2 But HE also from electromagnetic processes Synchrotron Inverse Compton
5 Detection Principle p, a m m p 3D PMT array m Cherenkov light from m m 42 Sea floor m m interaction The reconstruction is based on local coincidences compatible with the Cherenkov light front - Main channel: m interaction giving an ultra-relativistic m ( e and also) - Energy threshold ~ 20 GeV- 24hr operation, more than half sky coverage 5
6 Stockholm Physical Background sources Atmospheric muons: only downgoing Shield detector & reject downward goingmuons Atmospheric m 10 9 per year Atmospheric 10 4 per year Cosmic 0-10 per year? upgoing downgoing T. Chiarusi, M.S. Eur. Phys. Journal C (2010) arxiv:
7 The ANTARES Collaboration IFIC, Valencia UPV, Valencia UPC, Barcelona University of Erlangen NIKHEF, Bamberg Observatory Amsterdam Univ. of Wurzeburg Utrecht KVI Groningen NIOZ Texel ITEP,Moscow Moscow State Univ ISS, Bucarest CPPM, Marseille DSM/IRFU/CEA, Saclay APC, Paris LPC, Clermont-Ferrand IPHC, Strasbourg Univ. de H.-A., Mulhouse LAM, Marseille COM, Marseille GeoAzur Villefranche INSU-Division Technique LPRM, Oujda Univ./INFN of Bari Univ./INFN of Bologna Univ./INFN of Catania LNS Catania Univ./INFN of Pisa Univ./INFN of Rome Univ./INFN of Genova 8 countries 31 institutes ~150 scientists+engineers 7 7
8 The ANTARES Site & Infrastructure -2475m Shore Station IFREMER Toulon Centre 40 km submarine cable FOSELEV Marine 8
9 Stockholm The ANTARES Detector 2500m ~20 Mton instr vol inch PMTs 12 lines 25 storeys/line 3 PMTs / storey 450 m 40 km to shore Junction Box 70 m Interlink cables
10 : Building phase of the Detector ~70 m Junction box 2001 Main cable 2002 Line 1, Line 3, 4, 5 01 / 2007 Line 6, 7, 8, 9, / 2007 Line 11, /
11 Earth and Sea Sciences Connected 30 Oct 2010 Secondary Junction Box O2, CTD, P Seismograph Turbidity BioCam Currentmeter Instrumentation module 11
12 Up- and down-going Events reconstructed up-going neutrino detected in 6/12 detector lines: reconstructed down-going muon detected in all 12 detector lines: 12
13 Region of Sky Observable by Neutrino Telescopes IceCube (South Pole) ANTARES(43 North) Mkn 421 Mkn 501 Mkn 501 CRAB RX J CRAB SS433 SS433 GX339-4 VELA Galactic Centre Emphasis on study of Galactic sources 13
14 Selected ANTARES physics results 1. Cosmic sources searches 2. Diffuse flux from ExtraGalactic sources 3. Multimessenger approach and Gravitational Waves coincidences 4. Neutrino oscillations 14
15 1. Point Source Search Neutrino candidates: Upgoing particles Background for neutrinos: mis-reconstructed atmospheric muons Track fit quality used to reject mis-reconstructed downgoing muons Number of hits used as estimator of muon (~neutrino) energy upgoing Number of up-going events as a function of the track quality parameter L Angular distribution of wellreconstructed tracks 15
16 1. Angular Resolution for Neutrinos m Full 12 line detector cumulative distribution of the angle between the true neutrino track and the reconstructed muon event (assuming E -2 spectrum). The median is % of the events within 1 16
17 Stockholm 1. Full-Sky Search ( ) Sky map in equatorial coordinates (3058 candidates) Pre-trial prob Most significant cluster at: RA= 46.5, δ= ⁰ 3⁰. Results compatible with the background hypothesis N sig = 5 p-value=0.026 (post-trial) Significance = 2.2 σ
18 Stockholm 1. Source Candidate List Look in the direction of a list of 51 predefined candidate sources (selection of sources mostly based on γ-ray flux and visibility) First eleven sources sorted by p-value. Last column shows the 90% CL upper limit on the flux (E / GeV) -2 GeV -1 cm -2 s -1 HESS J most signal-like, p value 41% (post trial) Compatible with the background hypothesis
19 Stockholm 1. Candidate List Search 90%CL Limits ANTARES 2016 Assumes E -2 flux for a possible signal ANTARES has the most stringent limits for the Southern Sky Galactic sources expected to have energy cutoff- not visible to IceCube 2016: expect limits to improve by another factor ~2.5
20 2. Diffuse m flux Phys. Lett. B696 (2011) E 2 F(E) 90% = GeV cm -2 s -1 sr TeV<E<2.5 PeV IC40 20
21 2. Search for diffuse from Fermi Bubbles Fermi-LAT data provided evidence of the emission of HE rays with a high intensity E -2 spectrum from two large areas above and below the Galactic Center (the "Fermi bubbles"). A hadronic mechanism has been proposed for this rays emission making the Fermi bubbles promising sources of high-energy neutrinos For 100% hadronic models: E 2 df /de=1.2*10-7 GeV cm -2 s -1 sr -1 E cutoff protons: 1PeV-10 PeV Galactic coords Background estimated from average of three OFF regions (time shifted in local coordinates) Detector coords 21
22 2. Search for Neutrinos from Fermi Bubbles Live time = 588 days Cuts optimised for best MRF and a cutoff at 100 TeV ANTARES preliminary ON ZONE <OFF ZONE> N back (OFF) = 90±5(stat)±3(sys) N signal (ON) = 75 No signal exclude fully hadronic FB model without cutoff (90%CL F&C) Future: full dataset and improved energy estimator ANTARES preliminary 50 TeV cutoff 100 TeV cutoff 500 TeV cutoff no cutoff dotted: model prediction solid: 90% CL limits 22
23 3. Multimessenger approach Strategy: higher discovery potential by observing different probes higher significance by coincidence detection higher efficiency by relaxed cuts MoUs for joint research Alerts Ligo/Virgo Gravitational waves: trigger + dedicated analysis chain TAROT ROTSE optical follow up: arxiv: Astropart.Phys.35(2012) arxiv: GCN GRB Coord. Network: γ satellites arxiv:
24 3. Search for GW coincident signal V. V. Elewyck et al. Int.J.Mod.Phys. D18 (2009) B. Baret et al. Astropart.Phys. 35 (2011) 1-7 B. Baret et al. arxiv: Common data taking Search strategy Done On going Instantaneous Antares+Ligo+Virgo common view
25 Dataset Analysis set limits on distance of occurrence of NS-BH and NS-NS mergers Sub-optimal detectors No dedicated optimisation NO DETECTION Distance within which there is a 90% detection probability with a 1% false alarm rate per neutrino I. Di Palma et al. TAUP 2011 B. Bouhou et al. arxiv:
26 Stockholm 3. Correlation with Gravitational Waves - plausible common sources (microquasars, SGR, GRBs) - discovery potential for hidden sources (e.g. failed GRBs) 2007 ANTARES 5-line detector line detector adv LIGO/VRIGO 2007: No statistical significant correlation set limits on distance of occurrence of NS-BH and NS-NS mergers First joint ANTARES/LIGO/VIRGO publication: arxiv: v : expect to constrain fraction of star collapses accompanied by coincident emission of jets beamed towards Earth 26
27 Stockholm 4. Oscillations with Atmospheric Neutrinos L=2 R Earth cos, from track fit E from muon range E <100 GeV Oscillations maximal at E =24 GeV for vertical neutrinos Dashed line: oscillation effect Larger effect on single-line (low energy) than multi-line (higher energy) events MC truth 27
28 Stockholm 3. Neutrino Oscillations: Track Selection zenith angle resolution: 0.8 degrees for multi-line events 3 degrees for single-line events Multi-line Single-line Select pure sample of atmospheric neutrinos (<5% muon contamination) using a cut on the track fit quality Blue: misreconstructed atmospheric muons Green: atmospheric neutrinos Red: neutrino with oscillations
29 Stockholm 3. Neutrino Oscillations: Result data (863 days): No oscillation: 2 /NDF = 40/24 (2.1%) Best fit: 2 /NDF = 17.1/21 Δm 2 = ev 2 sin 2 2 =1.00 ANTARES preliminary no osc Systematics: (Absolute normalisation free) Absorption length: ±10% Detector efficiency: ±10% Spectral index of flux: ±0.03 OM angular acceptance ANTARES preliminary 68%CL contours 5% error on slope vs E R /cos R best osc ANTARES K2K Super-K MINOS Assuming maximal mixing: Δm 2 =(3.1±0.9) 10-3 ev 2 Accepted by PLB: arxiv:
30 Summary ANTARES infrastructure completed: Only operating deep sea neutrino telescope Largest neutrino telescope in the Northern hem. Operating smoothly, maintenance capability proven Good understanding of detector Important testbed for KM3NeT R&D and software Exciting and broad physics program. Unexplored regions of sensitivity for gal. sources Steady/transient sources, monopoles, DM, oscillations multi-messenger approach (optical, satellite, GW) Real-time readout and in-situ power capabilities a large program of multi-disciplinary activities: acoustics, biology, oceanography, seismology Major step towards the multi-kilometre cube deep-sea Neutrino telescope: KM3NeT 30
31 Spares 31
32 Counting Rates (short timescale) 2 min Continuous baseline: Radioactivity in the sea ( 40 K) + bioluminescent bacteria Bursts: bioluminescence from Macroscopic organisms 40 K K 20Ca e e 32
33 Acoustic Positioning Measure every 2 min: Distance line bases to 5 storeys/line and also storey headings and tilts Storey 1 Storey 8 Storey 14 Storey 20 Storey 25 Precision ~ few cms Radial displacement 33
34 Stockholm Absolute Pointing: Moon Shadow 884 days live time ( ) 2.7 sigma significance Agrees with Monte Carlo expectations 34
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 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 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 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 informationLATEST RESULTS OF THE ANTARES HIGH ENERGY NEUTRINO TELESCOPE
Torino - 13/07/2010 LATEST RESULTS OF THE ANTARES HIGH ENERGY NEUTRINO TELESCOPE Tommaso Chiarusi INFN - Sezione Bologna on behalf of the ANTARES Collaboration Physics with High Energy Cosmic νs SNR Binary
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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 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 informationOn the scientific motivation for a wide field-of-view TeV gamma-ray observatory in the Southern Hemisphere
On the scientific motivation for a wide field-of-view TeV gamma-ray observatory in the Southern Hemisphere for the HAWC collaboration E-mail: miguel@psu.edu Observations of high energy gamma rays are an
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 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 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 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 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 informationMulti-messenger studies of point sources using AMANDA/IceCube data and strategies
Multi-messenger studies of point sources using AMANDA/IceCube data and strategies Cherenkov 2005 27-29 April 2005 Palaiseau, France Contents: The AMANDA/IceCube detection principles Search for High Energy
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 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 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 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 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 informationGamma-ray Astrophysics
Gamma-ray Astrophysics AGN Pulsar SNR GRB Radio Galaxy The very high energy -ray sky NEPPSR 25 Aug. 2004 Many thanks to Rene Ong at UCLA Guy Blaylock U. of Massachusetts Why gamma rays? Extragalactic Background
More informationCherenkov Telescope Array Status Report. Salvatore Mangano (CIEMAT) On behalf of the CTA consortium
Cherenkov Telescope Array Status Report Salvatore Mangano (CIEMAT) On behalf of the CTA consortium Outline Very-High-Energy Gamma-Ray Astronomy Cherenkov Telescope Array (CTA) Expected Performance of CTA
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 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 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 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 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 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 informationMuon Reconstruction in IceCube
Muon Reconstruction in IceCube K.Hoshina for the IceCube collaboration June 26 2008 International workshop on High Energy Earth Science in Tokyo Introduction 2 IceCube is... A cubic-kilometer neutrino
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 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 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 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 informationANTARES. and the status of High-energy Neutrino Astronomy. Véronique Van Elewyck (APC & Université Paris Diderot)
ANTARES and the status of High-energy Neutrino Astronomy Véronique Van Elewyck (APC & Université Paris Diderot) Neutrino telescopes: why, how and where Limits on astrophysical and GZK neutrino fluxes Atmospheric
More informationCherenkov Telescope Array ELINA LINDFORS, TUORLA OBSERVATORY ON BEHALF OF CTA CONSORTIUM, TAUP
Cherenkov Telescope Array A SENSITIVE PROBE OF EXTREME UNIVERSE ELINA LINDFORS, TUORLA OBSERVATORY ON BEHALF OF CTA CONSORTIUM, TAUP 2015 1 The CTA Observatory SST ( 4m) LST ( 23m) MST ( 12m) South North
More informationMultimessenger test of Hadronic model for Fermi Bubbles Soebur Razzaque! University of Johannesburg
Multimessenger test of Hadronic model for Fermi Bubbles Soebur Razzaque! University of Johannesburg with! Cecilia Lunardini and Lili Yang Multi-messenger Astronomy 2 p π ±# ν# cosmic rays + neutrinos p
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 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 informationTHE EHE EVENT AND PROSPECTS FROM THE ICECUBE NEUTRINO OBSERVATORY. Lu Lu 千葉大
THE EHE EVENT 170922 AND PROSPECTS FROM THE ICECUBE NEUTRINO OBSERVATORY Lu Lu 千葉大 2 3 On-source n p TeV - PeV pp p n The Cosmic Neutrinos TeV->EeV p gp p n photopion production n GZK cosmogenic n EeV
More informationTime-dependent search of neutrino emission from X-ray and gamma-ray binaries with the ANTARES telescope
Time-dependent search of neutrino emission from X-ray and gamma-ray binaries with the ANTARES telescope A. Sánchez-Losa (INFN Sezione di Bari) D. Dornic (CPPM) A. Colerio (IFIC) agustin.sanchez@infn.ba.it
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 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 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 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 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 informationA New View of the High-Energy γ-ray Sky with the Fermi Telescope
A New View of the High-Energy γ-ray Sky with the Fermi Telescope Aurelien Bouvier KIPAC/SLAC, Stanford University On behalf of the Fermi collaboration SNOWPAC, 2010 The Fermi observatory Launch: June 11
More informationKM3NeT: Towards a km 3 Mediterranean Neutrino Telescope
2nd Workshop on Very Large Volume Neutrino Telescopes (VLVνT2), Catania, Sicily, November 8-11, 2005 KM3NeT: Towards a km 3 Mediterranean Neutrino Telescope Uli Katz Univ. Erlangen 09.11.2005 Some Physics
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 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 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 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 informationKM3NeT/ORCA. R. Bruijn University of Amsterdam/Nikhef. Phystat-Nu 2016 Tokyo
KM3NeT/ORCA R. Bruijn University of Amsterdam/Nikhef Phystat-Nu 2016 Tokyo 1 Overview Introduction KM3NeT & neutrino detection Main science goal: Neutrino mass hierarchy ORCA sensitivity study & detector
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 informationHigh Energy Emission. Brenda Dingus, LANL HAWC
High Energy Emission from GRBs Brenda Dingus, LANL HAWC What are GRBs? Cosmological distance Typical observed z>1 Energy released is up to few times the rest mass of Sun (if isotropic) in a few seconds
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 informationGravitational Waves and High Energy Neutrino coincidences : The gwhen Project
Gravitational Waves and High Energy Neutrino coincidences : The gwhen Project Thierry Pradier for the gwhen Group IPHC (IN2P3) & University of Strasbourg Antares : B. Baret, B. Bouhou, A. Kouchner, L.
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 informationFermi: Highlights of GeV Gamma-ray Astronomy
Fermi: Highlights of GeV Gamma-ray Astronomy Dave Thompson NASA GSFC On behalf of the Fermi Gamma-ray Space Telescope Large Area Telescope Collaboration Neutrino Oscillation Workshop Otranto, Lecce, Italy
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 informationCosmic Neutrinos in IceCube. Naoko Kurahashi Neilson University of Wisconsin, Madison IceCube Collaboration
Cosmic Neutrinos in IceCube Naoko Kurahashi Neilson University of Wisconsin, Madison IceCube Collaboration HEM KICP UChicago 6/9/2014 1 Outline IceCube capabilities The discovery analysis with updated
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 informationANTARES, KM3NeT, ORCA: Astronomy (and not only) in. the Abyss
trino Telescopes: w and the Next ade ANTARES, KM3NeT, ORCA: Astronomy (and not only) in ulti-tev and Beyond eudon, 30 Nov 2015 the Abyss Véronique Van Elewyck (APC & Université Paris Diderot) Paschal Coyle
More informationPreliminary results from gamma-ray observations with the CALorimeteric Electron Telescope (CALET)
Preliminary results from gamma-ray observations with the CALorimeteric Electron Telescope (CALET) Y.Asaoka for the CALET Collaboration RISE, Waseda University 2016/12/15 CTA-Japan Workshop The extreme
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 of the search for magnetic
Mohamed I University, Faculty of Sciences, Oujda Results of the search for magnetic monopoles with ANTARES Réunion du Groupement de Recherche sur les Neutrinos, Paris 29-30/05/2017 J. Brunner I. El Bojaddaini
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 informationConstraints on cosmic-ray origin from gamma-ray observations of supernova remnants
Constraints on cosmic-ray origin from gamma-ray observations of supernova remnants Marianne Lemoine-Goumard (CENBG, Université Bordeaux, CNRS-IN2P3, France) On behalf of the Fermi-LAT and HESS Collaborations
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 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 informationThe LHAASO-KM2A detector array and physical expectations. Reporter:Sha Wu Mentor: Huihai He and Songzhan Chen
The LHAASO-KM2A detector array and physical expectations Reporter:Sha Wu Mentor: Huihai He and Songzhan Chen Outline 1. Introduction 2. The KM2A Detector Array 3. Physical Expectations 3.1 Sensitivity
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 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 informationNeutrino Radiography of the Earth with the IceCube Neutrino Observatory
Neutrino Radiography of the Earth with the IceCube Neutrino Observatory Dec.4. 2012 AGU Fall Meeting 2012 in San Francisco Kotoyo Hoshina, Hiroyuki Tanaka and IceCube Collaboration Scan our Earth with
More informationIC59+40 Point Source Analysis. Mike Baker, Juan A Aguilar, Jon Dumm, Chad Finley, Naoko Kurahashi, Teresa Montaruli. 12 May 2011
IC59+40 Point Source Analysis Mike Baker, Juan A Aguilar, Jon Dumm, Chad Finley, Naoko Kurahashi, Teresa Montaruli 12 May 2011 http://wiki.icecube.wisc.edu/index.php/ic59+40_point_source_analysis Goals
More informationUnderstanding High Energy Neutrinos
Understanding High Energy Neutrinos Paolo Lipari: INFN Roma Sapienza NOW-2014 Conca Specchiulla 12th september 2014 An old dream is becoming a reality : Observing the Universe with Neutrinos ( A new way
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 informationANTARES sensitivity to steady cosmic gamma ray sources
ANTARES sensitivity to steady cosmic gamma ray sources G. Guillard To cite this version: G. Guillard. ANTARES sensitivity to steady cosmic gamma ray sources. ICRC011-3nd International Cosmic Ray Conference,
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 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 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 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 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 information