Characterization of Cryogenic Bolometers and Data Acquisition System for the CUORE Experiment
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The Gran Sasso Underground Laboratory Program
The Gran Sasso Underground Laboratory Program Eugenio Coccia INFN Gran Sasso and University of Rome “Tor Vergata” [email protected] XXXIII International Meeting on Fundamental Physics Benasque - March 7, 2005 Underground Laboratories Boulby UK Modane France Canfranc Spain INFN Gran Sasso National Laboratory LNGSLNGS ROME QuickTime™ and a Photo - JPEG decompressor are needed to see this picture. L’AQUILA Tunnel of 10.4 km TERAMO In 1979 A. Zichichi proposed to the Parliament the project of a large underground laboratory close to the Gran Sasso highway tunnel, then under construction In 1982 the Parliament approved the construction, finished in 1987 In 1989 the first experiment, MACRO, started taking data LABORATORI NAZIONALI DEL GRAN SASSO - INFN Largest underground laboratory for astroparticle physics 1400 m rock coverage cosmic µ reduction= 10–6 (1 /m2 h) underground area: 18 000 m2 external facilities Research lines easy access • Neutrino physics 756 scientists from 25 countries Permanent staff = 66 positions (mass, oscillations, stellar physics) • Dark matter • Nuclear reactions of astrophysics interest • Gravitational waves • Geophysics • Biology LNGS Users Foreigners: 356 from 24 countries Italians: 364 Permanent Staff: 64 people Administration Public relationships support Secretariats (visa, work permissions) Outreach Environmental issues Prevention, safety, security External facilities General, safety, electrical plants Civil works Chemistry Cryogenics Mechanical shop Electronics Computing and networks Offices Assembly halls Lab -
Annual Report 2009 P O R T
A LNGS/EXP-01/10 N May 2010 N U A L R E Annual Report 2009 P O R T 2 0 0 9 Lab ora tor i N o az s io as nal S i del Gran LNGS - s.s. 17 bis km 18,910 67010 ASSERGI (AQ) ITALY tel.+39 0862 4371 fax +39 0862 437559 email: [email protected] http://www.lngs.infn.it Codice ISBN ISBN-978-88-907304-5-0 Annual Report 2009 LNGS Director Dr. Lucia Votano Editor Dr. Roberta Antolini Technical Assistants Dr. Adriano Di Giovanni Marco Galeota The Gran Sasso National Laboratory My mandate as Director at LNGS took effect from September 2009 and it would be unthinkable to start this introduction to the 2009 LNGS annual report without mentioning the earthquake of last April which left 370 people dead, 15,000 injured and devastated the surrounding area together with the social and economic life of L’Aquila. Most of the lab personnel as well as the 70,000 inhabitants in L’Aquila were rendered homeless. Fortunately the Laboratory survived the devastating earthquake and escaped damage. This was possible thanks to two factors: the acceleration experienced deep underground, (0.03g), as expected, was lower than that of the external laboratory (0.15 g) and much lower than in L’Aquila (0.64 g).; the anti-seismic design of the apparatus protected the underground installations. In April Eugenio Coccia was still on duty as Director of the Lab, and I think it is proper to mention how effective his dedication and actions were, in providing support to the laboratory personnel and assuring the immediate restarting of the activities in the Laboratory. -
Required Sensitivity to Search the Neutrinoless Double Beta Decay in 124Sn
Required sensitivity to search the neutrinoless double beta decay in 124Sn Manoj Kumar Singh,1;2∗ Lakhwinder Singh,1;2 Vivek Sharma,1;2 Manoj Kumar Singh,1 Abhishek Kumar,1 Akash Pandey,1 Venktesh Singh,1∗ Henry Tsz-King Wong2 1 Department of Physics, Institute of Science, Banaras Hindu University, Varanasi 221005, India. 2 Institute of Physics, Academia Sinica, Taipei 11529, Taiwan. E-mail: ∗ [email protected] E-mail: ∗ [email protected] Abstract. The INdias TIN (TIN.TIN) detector is under development in the search for neutrinoless double-β decay (0νββ) using 90% enriched 124Sn isotope as the target mass. This detector will be housed in the upcoming underground facility of the India based Neutrino Observatory. We present the most important experimental parameters that would be used in the study of required sensitivity for the TIN.TIN experiment to probe the neutrino mass hierarchy. The sensitivity of the TIN.TIN detector in the presence of sole two neutrino double-β decay (2νββ) decay background is studied at various energy resolutions. The most optimistic and pessimistic scenario to probe the neutrino mass hierarchy at 3σ sensitivity level and 90% C.L. is also discussed. Keywords: Double Beta Decay, Nuclear Matrix Element, Neutrino Mass Hierarchy. arXiv:1802.04484v2 [hep-ph] 25 Oct 2018 PACS numbers: 12.60.Fr, 11.15.Ex, 23.40-s, 14.60.Pq Required sensitivity to search the neutrinoless double beta decay in 124Sn 2 1. Introduction Neutrinoless double-β decay (0νββ) is an interesting venue to look for the most important question whether neutrinos have Majorana or Dirac nature. -
Nuclear Physics
Nuclear Physics Overview One of the enduring mysteries of the universe is the nature of matter—what are its basic constituents and how do they interact to form the properties we observe? The largest contribution by far to the mass of the visible matter we are familiar with comes from protons and heavier nuclei. The mission of the Nuclear Physics (NP) program is to discover, explore, and understand all forms of nuclear matter. Although the fundamental particles that compose nuclear matter—quarks and gluons—are themselves relatively well understood, exactly how they interact and combine to form the different types of matter observed in the universe today and during its evolution remains largely unknown. Nuclear physicists seek to understand not just the familiar forms of matter we see around us, but also exotic forms such as those that existed in the first moments after the Big Bang and that exist today inside neutron stars, and to understand why matter takes on the specific forms now observed in nature. Nuclear physics addresses three broad, yet tightly interrelated, scientific thrusts: Quantum Chromodynamics (QCD); Nuclei and Nuclear Astrophysics; and Fundamental Symmetries: . QCD seeks to develop a complete understanding of how the fundamental particles that compose nuclear matter, the quarks and gluons, assemble themselves into composite nuclear particles such as protons and neutrons, how nuclear forces arise between these composite particles that lead to nuclei, and how novel forms of bulk, strongly interacting matter behave, such as the quark-gluon plasma that formed in the early universe. Nuclei and Nuclear Astrophysics seeks to understand how protons and neutrons combine to form atomic nuclei, including some now being observed for the first time, and how these nuclei have arisen during the 13.8 billion years since the birth of the cosmos. -
THE BOREXINO IMPACT in the GLOBAL ANALYSIS of NEUTRINO DATA Settore Scientifico Disciplinare FIS/04
UNIVERSITA’ DEGLI STUDI DI MILANO DIPARTIMENTO DI FISICA SCUOLA DI DOTTORATO IN FISICA, ASTROFISICA E FISICA APPLICATA CICLO XXIV THE BOREXINO IMPACT IN THE GLOBAL ANALYSIS OF NEUTRINO DATA Settore Scientifico Disciplinare FIS/04 Tesi di Dottorato di: Alessandra Carlotta Re Tutore: Prof.ssa Emanuela Meroni Coordinatore: Prof. Marco Bersanelli Anno Accademico 2010-2011 Contents Introduction1 1 Neutrino Physics3 1.1 Neutrinos in the Standard Model . .4 1.2 Massive neutrinos . .7 1.3 Solar Neutrinos . .8 1.3.1 pp chain . .9 1.3.2 CNO chain . 13 1.3.3 The Standard Solar Model . 13 1.4 Other sources of neutrinos . 17 1.5 Neutrino Oscillation . 18 1.5.1 Vacuum oscillations . 20 1.5.2 Matter-enhanced oscillations . 22 1.5.3 The MSW effect for solar neutrinos . 26 1.6 Solar neutrino experiments . 28 1.7 Reactor neutrino experiments . 33 1.8 The global analysis of neutrino data . 34 2 The Borexino experiment 37 2.1 The LNGS underground laboratory . 38 2.2 The detector design . 40 2.3 Signal processing and Data Acquisition System . 44 2.4 Calibration and monitoring . 45 2.5 Neutrino detection in Borexino . 47 2.5.1 Neutrino scattering cross-section . 48 2.6 7Be solar neutrino . 48 2.6.1 Seasonal variations . 50 2.7 Radioactive backgrounds in Borexino . 51 I CONTENTS 2.7.1 External backgrounds . 53 2.7.2 Internal backgrounds . 54 2.8 Physics goals and achieved results . 57 2.8.1 7Be solar neutrino flux measurement . 57 2.8.2 The day-night asymmetry measurement . 58 2.8.3 8B neutrino flux measurement . -
RES-NOVA Sensitivity to Core-Collapse and Failed Core-Collapse Supernova Neutrinos
Prepared for submission to JCAP RES-NOVA sensitivity to core-collapse and failed core-collapse supernova neutrinos L. Pattavinaa;b;1 N. Ferreiro Iachellinic;1 L. Pagnaninia;d L. Canonicac E. Celib;d M. Clemenzae F. Ferronid;f E. Fiorinie A. Garaic L. Gironie M. Mancusoc S. Nisia F. Petriccac S. Pirroa S. Pozzie A. Puiua;d J. Rotheb S. Schönertb L. Shtembaric R. Straussb V. Wagnerb aINFN Laboratori Nazionali del Gran Sasso, 67100 Assergi, Italy bPhysik-Department and Excellence Cluster Origins, Technische Universität München, 85747 Garching, Germany arXiv:2103.08672v2 [astro-ph.IM] 16 Aug 2021 cMax-Planck-Institut für Physik, 80805 München, Germany dGran Sasso Science Institute, 67100, L’Aquila, Italy eINFN Sezione Milano - Bicocca and Dipartimento di Fisica, Università di Milano - Bicocca, 20126 Milano, Italy f INFN Sezione di Roma1, 00185, Roma, Italy 1Corresponding authors. E-mail: [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], ettore.fi[email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected] Abstract. RES-NOVA is a new proposed experiment for the investigation of astrophysical neutrino sources with archaeological Pb-based cryogenic detectors. RES-NOVA will exploit Coherent Elastic neutrino-Nucleus Scattering (CEνNS) as detection channel, thus it will be equally sensitive to all neutrino flavors produced by Supernovae (SNe). -
Arxiv:1904.01056V1 [Physics.Ins-Det] 1 Apr 2019 ‡ † ∗ Acltos Cosawd Nryrneadi Various [5–7]
APS/IOA-165 3 Simulated neutrino signals of low and intermediate energy neutrinos on Cd detectors J. Sinatkas∗ Department of Informatics Engineering, Technological Institute of Western Macedonia, Kastoria, GR-52100 V. Tsakstara† Electrical Engineering Department, Technological Institute of Western Macedonia, School of Applied Science,Kozani, GR-50100 and Division of Theoretical Physics, University of Ioannina, GR-45110 Ioannina, Greece Odysseas Kosmas‡ Modelling and Simulation Centre, MACE, University of Manchester, Sackville Street, Manchester, UK (Dated: April 3, 2019) Neutrino-nucleus reactions cross sections, obtained for neutrino energies in the range εν ≤ 100 − 120 MeV (low- and intermediate-energy range), which refer to promising neutrino detec- tion targets of current terrestrial neutrino experiments, are presented and discussed. At first, we evaluated original cross sections for elastic scattering of neutrinos produced from various astrophys- ical and laboratory neutrino sources with the most abundant Cd isotopes 112Cd, 114Cd and 116Cd. These isotopes constitute the main material of the COBRA detector aiming to search for neutrino- less double beta decay events and neutrino-nucleus scattering events at the Gran Sasso laboratory (LNGS). The coherent ν-nucleus reaction channel addressed with emphasis here, dominates the neutral current ν-nucleus scattering, events of which have only recently been observed for a first time in the COHERENT experiment at Oak Ridge. Subsequently, simulated ν-signals expected to be recorded at Cd detectors are derived through the application of modern simulation techniques and employment of reliable neutrino distributions of astrophysical ν-sources (as the solar, super- nova and Earth neutrinos), as well as laboratory neutrinos (like the reactor neutrinos, the neutrinos produced from pion-muon decay at rest and the β-beam neutrinos produced from the acceleration of radioactive isotopes at storage rings as e.g. -
Full TIPP 2011 Program Book
Second International Conference on Technology and Instrumentation in Particle Physics June 9-14, 2011 Program & Abstracts Sheraton Chicago Hotel and Towers, Chicago IL ii TIPP 2011 — June 9-14, 2011 Table of Contents Acknowledgements .................................................................................................................................... v Session Conveners ...................................................................................................................................vii Session Chairs .......................................................................................................................................... ix Agenda ....................................................................................................................................................... 1 Abstracts .................................................................................................................................................. 35 Poster Abstracts ..................................................................................................................................... 197 Abstract Index ........................................................................................................................................ 231 Poster Index ........................................................................................................................................... 247 Author List ............................................................................................................................................. -
Status and Outlook of the CUORE and CUPID Experimental Calorimetry Programs: an Overview
Status and Outlook of the CUORE and CUPID Experimental Calorimetry Programs: An Overview Danielle H. Speller for the CUORE and CUPID Collaborations Johns Hopkins University August 5, 2020 Slides provided by CUORE, CUPID, CUPID‐Mo, and Acknowledgements CUPID‐0 Collaborations 8/5/2020 Danielle H. Speller (JHU), CUORE/CUPID, Snowmass Neutrino Workshop 2 Searching for Neutrinoless Double‐Beta Decay with CUORE CUORE: The Cryogenic Underground Observatory for Rare Events • The first tonne‐scale 0νββ experiment operating with thermal detectors • Main objective: 0νββ in 130Te 3 • 988 TeO2 crystals, 5×5×5 cm each • Total mass: 742 kg TeO2 • 130Te mass: 206 kg (all natural abundance) • Macrocalorimeter operation in ~10 mK cryostat Heat bath ~10 mK Thermistor (NTD-Ge) • Located underground at LNGS (Italy) (Copper) • Expected energy resolution at 2615 keV: 5 keV Absorber Crystal (TeO2) FWHM • Background goal: 0.01 cts/(keV∙kg ∙yr) at Qββ 0ν 25 • Sensitivity: T1/2 = 9×10 yr (90% C.I.) in 5 Energy Cryogenics 102, 9‐21 (2019). Thermal coupling release arxiv:1904.05745 years of data collection (Eur. Phys. J. C (2017) (PTFE) Cryogenics 93, 56‐65 (2018). 77:532) arxiv:1712.02753 Danielle H. Speller (JHU), CUORE/CUPID, Snowmass Neutrino 8/5/2020 3 Workshop • Total analyzed exposure: region of interest Recent Results: Improved 372.5 kg∙yr • Median exclusion sensitivity: • Resolution (expo.‐weighted 1.7 x 1025 yr 130 harmonic avg, Qββ): 7.0±0.4 0ν 25 • T1/2 > 3.2 x 10 yr (90% C.I.) Limit on 0νββ in Te with keV Bayesian lower limit on 130Te • Background: 1.38±0.07 x 10‐2 half‐life CUORE (2020) cts/(keV∙kg∙yr) in the 0νββ Phys. -
Neutrinoless Double Beta Decay Searches
FLASY2019: 8th Workshop on Flavor Symmetries and Consequences in 2016 Symmetry Magazine Accelerators and Cosmology Neutrinoless Double Beta Decay Ke Han (韩柯) Shanghai Jiao Tong University Searches: Status and Prospects 07/18, 2019 Outline .General considerations for NLDBD experiments .Current status and plans for NLDBD searches worldwide .Opportunities at CJPL-II NLDBD proposals in China PandaX series experiments for NLDBD of 136Xe 07/22/19 KE HAN (SJTU), FLASY2019 2 Majorana neutrino and NLDBD From Physics World 1935, Goeppert-Mayer 1937, Majorana 1939, Furry Two-Neutrino double beta decay Majorana Neutrino Neutrinoless double beta decay NLDBD 1930, Pauli 1933, Fermi + 2 + (2 ) Idea of neutrino Beta decay theory 136 136 − 07/22/19 54 → KE56 HAN (SJTU), FLASY2019 3 ̅ NLDBD probes the nature of neutrinos . Majorana or Dirac . Lepton number violation . Measures effective Majorana mass: relate 0νββ to the neutrino oscillation physics Normal Inverted Phase space factor Current Experiments Nuclear matrix element Effective Majorana neutrino mass: 07/22/19 KE HAN (SJTU), FLASY2019 4 Detection of double beta decay . Examples: . Measure energies of emitted electrons + 2 + (2 ) . Electron tracks are a huge plus 136 136 − 54 → 56 + 2 + (2)̅ . Daughter nuclei identification 130 130 − 52 → 54 ̅ 2νββ 0νββ T-REX: arXiv:1512.07926 Sum of two electrons energy Simulated track of 0νββ in high pressure Xe 07/22/19 KE HAN (SJTU), FLASY2019 5 Impressive experimental progress . ~100 kg of isotopes . ~100-person collaborations . Deep underground . Shielding + clean detector 1E+27 1E+25 1E+23 1E+21 life limit (year) life - 1E+19 half 1E+17 Sn Ca νββ Ge Te 0 1E+15 Xe 1E+13 1940 1950 1960 1970 1980 1990 2000 2010 2020 Year . -
The World Underground Scientific Facilities a Compendium
A. Bettini G. Galilei Physics Department. Padua University INFN. Padua Canfranc Underground Laboratory [email protected] THE WORLD UNDERGROUND SCIENTIFIC FACILITIES A COMPENDIUM Abstract. Underground laboratories provide the low radioactive background environment necessary to explore the highest energy scales that cannot be reached with accelerators, by searching for extremely rare phenomena. I have requested to the Directors of the Laboratories a standard set of questions on the principal characteristics of their laboratory and collected them in this compendium. I included the ideas and plans for short-range developments. However, next-generation structures, such as those for megaton-size detectors, are not discussed. A short version of this work will be published in the Proccedings of TAUP 2007. 1 2 PREFACE . 4 EUROPE...................................................................................................................................... 6 BNO. BAKSAN NEUTRINO OBSERVATORY (RUSSIA)............................................................................ 6 BUL. BOULBY PALMER LABORATORY (UK)....................................................................................... 9 CUPP. CENTRE FOR UNDERGROUND PHYSICS AT PYHÄSALMI (FINLAND)............................................ 11 LNGS. LABORATORI NAZIONALI DEL GRAN SASSO. L’AQUILA (ITALY) ............................................... 13 LSC. LABORATORIO SUBTERRÁNEO DE CANFRANC (SPAIN).............................................................. 16 LSM. LABORATOIRE -
The COBRA Experiment
10th Int. Conf. on Topics in Astroparticle and Underground Physics (TAUP2007) IOP Publishing Journal of Physics: Conference Series 120 (2008) 052048 doi:10.1088/1742-6596/120/5/052048 The COBRA Experiment 1J.R. Wilson2 Department of Physics and Astronomy, University of Sussex, Brighton, BN1 9QH, UK E-mail: [email protected] Abstract. The COBRA experiment aims to use a large array of CdZnTe semiconductor detectors to search for neutrinoless double beta decay. The COBRA collaboration are currently operating a small proto-type array of crystals in a low-background environment. This paper presents the current status of the experiment, results from current and previous proto-types and future prospects for COBRA. 1. Concept COBRA aims to search for neutrinoless double beta decay (0νββ) in CdZnTe semiconductor crystals[1]. There are actually 9 candidate 0νββ isotopes, 5 in the form of β −β− emitters, intrinsic to the detector material, but measurements will focus on 116Cd. This has the highest Q-value at 2.8 MeV, beyond all the single gamma-lines from the natural decay chains which would be problematic in contaminating signal regions at lower energies. CdZnTe, in common with other semiconductors, can be produced cleanly with low levels of intrinsic radioactive background and offers good energy resolution. Unlike many semiconductors though, CdZnTe can be operated at room temperature without the need for expensive cryogenics close to the detectors. For a neutrino mass of about 50 meV, as suggested by neutrino oscillation data, the half-life of 116Cd is of order 1026 years (exact values depend on the nuclear matrix elements).