The Miniboone Experiment
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Arxiv:1812.08768V2 [Hep-Ph] 3 Dec 2019
IPPP/18/113/FERMILAB-PUB-18-686-A-ND-PPD-T Testing New Physics Explanations of MiniBooNE Anomaly at Neutrino Scattering Experiments 1, 2, 3, Carlos A. Argüelles, ∗ Matheus Hostert, y and Yu-Dai Tsai z 1Dept. of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA 2Institute for Particle Physics Phenomenology, Department of Physics, Durham University, South Road, Durham DH1 3LE, United Kingdom 3Fermilab, Fermi National Accelerator Laboratory, Batavia, IL 60510, USA (Dated: December 5, 2019) Heavy neutrinos with additional interactions have recently been proposed as an explanation to the MiniBooNE excess. These scenarios often rely on marginally boosted particles to explain the excess angular spectrum, thus predicting large rates at higher-energy neutrino-electron scattering experiments. We place new constraints on this class of models based on neutrino-electron scattering sideband measurements performed at MINERνA and CHARM-II. A simultaneous explanation of the angular and energy distributions of the MiniBooNE excess in terms of heavy neutrinos with light mediators is severely constrained by our analysis. In general, high-energy neutrino-electron scattering experiments provide strong constraints on explanations of the MiniBooNE observation involving light mediators. Introduction – Non-zero neutrino masses have been the experiment has observed an excess of νe-like events established in the last twenty years by measurements of that is currently in tension with the standard three- neutrino flavor conversion in natural and human-made neutrino prediction and is beyond statistical doubt at the sources, including long- and short-baseline experiments. 4:7σ level [5]. While it is possible that the excess is fully The overwhelming majority of data supports the three- or partially due to systematic uncertainties or SM back- neutrino framework. -
Miniboone Anomaly and Nuclear Physics 4
1. MiniBooNE 2. Beam 3. Detector MiniBooNE Anomaly and Nuclear physics 4. Oscillation 5. Discussion PRL121(2018)221801 outline 1. MiniBooNE neutrino experiment 2. Nucleon correlations 3. Pion puzzle 4. NC single photon production 5. Conclusions Teppei Katori Queen Mary University of London ECT* workshop, Trento, Italy, April 15, 2019 Teppei Katori, [email protected] 15/04/19 1 1. MiniBooNE 2. Beam 3. Detector 4. Oscillation 5. Discussion 1. MiniBooNE neutrino experiment 2. Nucleon correlations 3. Pion puzzle 4. NC single photon production 5. Discussions Teppei Katori, [email protected] 15/04/19 2 1. MiniBooNE 2. Beam 3. Detector 4. Oscillation 5. Discussion Teppei Katori, [email protected] 15/04/19 3 1. MiniBooNE 2. Beam 3. Detector 4. Oscillation 5. Discussion The most visible particle physics result of the year Teppei Katori, [email protected] 15/04/19 4 https://physics.aps.org/articles/v11/122 PHYSICAL REVIEW LETTERS 120, 141802 (2018) signature of dark matter annihilation in the Sun [5,6]. 1. MiniBooNE Despite the importance of the KDAR neutrino, it has never MiniBooNE 2. Beam been isolated and identified. 3. Detector 86 m 4. Oscillation In the charged current (CC) interaction of a 236 MeV νμ background KDAR 12 − NuMI 5. Discussion (νμ C → μ X), the muon kinetic energy (Tμ) and closely beam decay pipe related neutrino-nucleus energy transfer (ω E − E ) horns ν μ target distributions are of particular interest for benchmarking¼ absorber neutrino interaction models and generators, which report widely varying predictions for kinematics at these tran- 5 m 675 m sition-region energies [7–14]. -
Icecube Searches for Neutrinos from Dark Matter Annihilations in the Sun and Cosmic Accelerators
UNIVERSITE´ DE GENEVE` FACULTE´ DES SCIENCES Section de physique Professeur Teresa Montaruli D´epartement de physique nucl´eaireet corpusculaire IceCube searches for neutrinos from dark matter annihilations in the Sun and cosmic accelerators. THESE` pr´esent´ee`ala Facult´edes sciences de l'Universit´ede Gen`eve pour obtenir le grade de Docteur `essciences, mention physique par M. Rameez de Kozhikode, Kerala (India) Th`eseN◦ 4923 GENEVE` 2016 i Declaration of Authorship I, Mohamed Rameez, declare that this thesis titled, 'IceCube searches for neutrinos from dark matter annihilations in the Sun and cosmic accelerators.' and the work presented in it are my own. I confirm that: This work was done wholly or mainly while in candidature for a research degree at this University. Where any part of this thesis has previously been submitted for a degree or any other qualifica- tion at this University or any other institution, this has been clearly stated. Where I have consulted the published work of others, this is always clearly attributed. Where I have quoted from the work of others, the source is always given. With the exception of such quotations, this thesis is entirely my own work. I have acknowledged all main sources of help. Where the thesis is based on work done by myself jointly with others, I have made clear exactly what was done by others and what I have contributed myself. Signed: Date: 27 April 2016 ii UNIVERSITE´ DE GENEVE` Abstract Section de Physique D´epartement de physique nucl´eaireet corpusculaire Doctor of Philosophy IceCube searches for neutrinos from dark matter annihilations in the Sun and cosmic accelerators. -
Icecube Sterile Neutrino Searches
EPJ Web of Conferences 207, 04005 (2019) https://doi.org/10.1051/epjconf/201920704005 VLVnT-2018 IceCube Sterile Neutrino Searches 1, B.J.P. Jones ∗ For the IceCube Collaboration 1University of Texas at Arlington, 108 Science Hall, 502 Yates St, Arlington, TX Abstract. Anomalies in short baseline experiments have been interpreted as evidence for additional neutrino mass states with large mass splittings from the known, active flavors. This explanation mandates a corresponding signa- ture in the muon neutrino disappearance channel, which has yet to be observed. Searches for muon neutrino disappearance at the IceCube neutrino telescope presently provide the strongest limits in the space of mixing angles for eV- scale sterile neutrinos. This proceeding for the Very Large Volume Neutrino Telescopes (VLVnT) Workshop summarizes the IceCube analyses that have searched for sterile neutrinos and describes ongoing work toward enhanced, high-statistics sterile neutrino searches. 1 Introduction Sterile neutrinos are hypothetical particles that have been invoked to explain anomalies in short baseline accelerator decay-at-rest [1] and decay-in-flight experiments [2], reactor neu- trino fluxes [3, 4] and radioactive source experiments [5]. In low-energy, short baseline exper- iments that are sensitive to νe appearance, matter effects can be neglected and an oscillation of the form: 2 2 2 ∆m L Pν ν = sin 2θµe sin (1) µ→ e 4E is predicted. A large ∆m2 thus introduces an oscillation at a small characteristic L/E, with 2 the effective mixing parameter, sin 2θµe governing the amplitude of oscillation. To introduce flavor-change at similar L/E as exhibited in the MiniBooNE and LSND experiments, mixing 2 3 parameters sin 2θµe of 10− or larger are required, with favored parameter space in the one- to-few eV2 mass splittings. -
Current Status of Neutrino Anomalies
Current Status of Neutrino Anomalies Srubabati Goswami Physical Research Laboratory, Ahmedabad, India Anomalies 2020 !1 Is it a monument, a madrasa or a market square? Charminar holds many mysteries within its fold https://www.thehindu.com/society/history-and-culture/the-very-many-mysteries-of-hyderabads-charminar/ article24311906.ece !2 Neutrino: many questions ❖ What Unknown oscillation parameters - hierarchy, octant of 2-3 mixing angle and CP phase ❖ Absolute neutrino masses — beta decay, cosmology ❖ Nature of neutrinos - Dirac or Majorana — neutrino less double beta decay ❖ Are there more than three flavours — sterile neutrinos ❖ Origin of neutrino masses and mixing — seesaw , flavour symmetry — physics beyond Standard Model !3 Neutrino Connections Baryogenesis via Collider leptogenesis Physics Dark Matter Higgs/Vacuum Cosmology stability Neutrinos Astrophysics/ CLFV Multimessenger Nucl. Physics/ interactions !4 Plan of talk New physics Neutrino Neutrinoless Ultra high In neutrino Oscillation double Energy neutrinos Parameters oscillation beta decay NSI Sterile Nus !5 Neutrino Oscillations Solar Atmospheric Reactor Accelerator !6 New result from Borexino !7 First detection of CNO neutrinos R(CNO) = 7.2 +2.9 -1.7 cpd/100ton Null hypothesis(CNO=0) rejected at 5.1 sigma. G. Ranucci , Neutrino 2020 !8 Three Neutrino Paradigm ❖ Measurement of non-zero in reactor experiments three neutrino picture !9 NOvA Results Joint analysis of disappearance and Appearance data in both neutrino and antineutrino channel ❖ P Preference for Neutrino 2020 !10 -
Measurement of the + ̅ Charged Current Inclusive Cross Section
Measurement of the �! + �!̅ Charged Current Inclusive Cross Section on Argon in MicroBooNE Krishan Mistry on behalf of the MicroBooNE Collaboration 15 March 2021 New Directions in Neutrino-Nucleus Scattering (NDNN) NuSTEC Workshop ICARUS T600 MicroBooNE SBND Importance of the �!-Ar cross section • MicroBooNE + SBN Program + DUNE ⇥ Employ Liquid Argon Time Projection Chambers (LArTPCs) arXiv:1503.01520 [physics.ins-det] • Primary signal channel for these experiments is �!– Ar CC interactions arXiv:2002.03005 [hep-ex] 15 March 2021 K Mistry 2 Building a Picture of �! Interactions ArgoNeuT is the first A handful of measurements measurement made on on other nuclei in the argon hundred MeV to GeV range ⇥ Sample of 13 selected events Nuclear Physics B 133, 205 – 219 (1978) Phys. Rev. D 102, 011101(R) (2020) ⇥ Gargamelle Phys. Rev. Lett. 113, 241803 (2014) ⇥ Phys. Rev. D 91, 112010 (2015) T2K J. High Energ. Phys. 2020, 114 (2020) ⇥ MINER�A Phys. Rev. Lett. 116, 081802 (2016) !! " !! " Argon Other 15 March 2021 K Mistry 3 What are we measuring? ! /!̅ " # • Total �!+ �!̅ Charged Current (CC) ! ! $ /$ inclusive cross section • Signature: the neutrino event ? contains at least one electron-liKe shower Ar ⇥ No requirements on the presence (or absence) of any additional particle ⇥ Do not differentiate between �! and �!̅ Inclusive channel is the most straightforward channel to compare to predictions 15 March 2021 K Mistry 4 MicroBooNE • Measurement is performed • Features of a LArTPC using the MicroBooNE detector: LArTPC ⇥ Precise calorimetry ⇥ 4� -
First MINOS Results from the Numi Beam Nathaniel Tagg, for the MINOS Collaboration Tufts University, 4 Colby Street, Medford, MA, USA 02155 FERMILAB-CONF-06-130-E
First MINOS Results from the NuMI Beam Nathaniel Tagg, for the MINOS Collaboration Tufts University, 4 Colby Street, Medford, MA, USA 02155 FERMILAB-CONF-06-130-E As of December 2005, the MINOS long-baseline neutrino oscillation experiment collected data with an exposure of 0.93 × 1020 protons on target. Preliminary analysis of these data reveals a result inconsistent with a no- oscillation hypothesis at level of 5.8 sigma. The data are consistent with neutrino oscillations reported by m2 . +0.60 × − 2 θ . +0.12 Super-Kamiokande and K2K, with best fit parameters of ∆ 23 = 3 05−0.55 10 3 and sin 2 23 = 0 88−0.15. 1. Introduction end of the run period in March 2006, the maximum in- tensity delivered to the target was in excess of 25 1012 × The MINOS long-baseline neutrino oscillation ex- protons per pulse, with a maximum target power of periment [1] was designed to accurately measure neu- 250 kW. trino oscillation parameters by looking for νµ disap- pearance. MINOS will improve the measurements of ∆m223 first performed by the Super-Kamiokande 3. The MINOS Detectors [2, 3] and K2K experiments [4]. In addition, MINOS is capable of searching for sub-dominant νµ νe os- The MINOS Near and Far detectors are constructed cillations, can look for CPT-violating modes→ by com- to have nearly identical composition and cross-section. paring νµ toν ¯µ oscillations, and is used to observe The detectors consist of sandwiches of 2.54 cm thick atmospheric neutrinos [5]. steel and 1 cm thick plastic scintillator, hung verti- The MINOS experiment uses a beam of νµ created cally. -
“ Chamber” Neutrino Physi Years After Gargamelle
35 years after Gargamelle: the Renaissance of the “ Bubble chamber” neutrino physics Carlo Rubbia CERN, Geneva, Switzerland INFN-Assergi, Italy C. Rubbia, CERN, 0ct09 111 A Gargamelle neutrino event QuickTime™ and a decompressor are needed to see this picture. Charm production in a neutrino interaction The total visible energy is 3.58 GeV. C. Rubbia, CERN, 0ct09 Slide: 2 The path to massive liquid Argon detectors CERN 1 2 Laboratory work CERN CERN 3 T600 detector 4 2001: First T600 module 5 20 m Cooperation with industry C. Rubbia, CERN, 0ct09 Slide: 3 T600 in hall B (CNGS2 -2009) QuickTime™ and a decompressor are needed to see this picture. C. Rubbia, CERN, 0ct09 Slide: 4 Thirty years of progress........ LAr is a cheap liquid Bubble diameter ≈ 3 mm (≈1CHF/litre), vastly (diffraction limited) produced by industry Gargamelle bubble chamber ICARUS electronic chamber “Bubble” size 3 x 3 x 0.3 mm3 T300 real event Medium Heavy freon Medium Liquid Argon Sensitive mass 3.0 ton Sensitive mass Many ktons Density 1.5 g/cm3 Density 1.4 g/cm3 Radiation length 11.0 cm Radiation length 14.0 cm Collision length 49.5 cm Collision length 54.8 cm dE/dx 2.3 MeV/cm dE/dx 2.1 MeV/cm C. Rubbia, CERN, 0ct09 Slide: 5 Summary of LAr TPC performances l Tracking device ØPrecise event topology ØMomentum via multiple scattering l Measurement of local energy deposition dE/dx T300 real event Øe / γ separation (2%X 0 sampling) ØParticle ID by means of dE/dx vs range l Total energy reconstruction of the events from charge integration ØFull sampling, homogeneous calorimeter with excellent accuracy for contained events RESOLUTIONS Low energy electrons: σ(E)/E = 11% / √ E(MeV)+2% Electromagn. -
Alpha Backgrounds and Their Implications for Neutrinoless Double-Beta Decay Experiments Using Hpge Detectors
Alpha Backgrounds and Their Implications for Neutrinoless Double-Beta Decay Experiments Using HPGe Detectors Robert A. Johnson A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Washington 2010 Program Authorized to Offer Degree: Physics University of Washington Graduate School This is to certify that I have examined this copy of a doctoral dissertation by Robert A. Johnson and have found that it is complete and satisfactory in all respects, and that any and all revisions required by the final examining committee have been made. Chair of the Supervisory Committee: John F. Wilkerson Reading Committee: Steven R. Elliott Nikolai R. Tolich John F. Wilkerson Date: In presenting this dissertation in partial fulfillment of the requirements for the doctoral degree at the University of Washington, I agree that the Library shall make its copies freely available for inspection. I further agree that extensive copying of this dissertation is allowable only for scholarly purposes, consistent with “fair use” as prescribed in the U.S. Copyright Law. Requests for copying or reproduction of this dissertation may be referred to Proquest Information and Learning, 300 North Zeeb Road, Ann Arbor, MI 48106-1346, 1-800-521-0600, to whom the author has granted “the right to reproduce and sell (a) copies of the manuscript in microform and/or (b) printed copies of the manuscript made from microform.” Signature Date University of Washington Abstract Alpha Backgrounds and Their Implications for Neutrinoless Double-Beta Decay Experiments Using HPGe Detectors Robert A. Johnson Chair of the Supervisory Committee: Professor John F. -
INO/ICAL/PHY/NOTE/2015-01 Arxiv:1505.07380 [Physics.Ins-Det]
INO/ICAL/PHY/NOTE/2015-01 ArXiv:1505.07380 [physics.ins-det] Pramana - J Phys (2017) 88 : 79 doi:10.1007/s12043-017-1373-4 Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO) The ICAL Collaboration arXiv:1505.07380v2 [physics.ins-det] 9 May 2017 Physics Potential of ICAL at INO [The ICAL Collaboration] Shakeel Ahmed, M. Sajjad Athar, Rashid Hasan, Mohammad Salim, S. K. Singh Aligarh Muslim University, Aligarh 202001, India S. S. R. Inbanathan The American College, Madurai 625002, India Venktesh Singh, V. S. Subrahmanyam Banaras Hindu University, Varanasi 221005, India Shiba Prasad BeheraHB, Vinay B. Chandratre, Nitali DashHB, Vivek M. DatarVD, V. K. S. KashyapHB, Ajit K. Mohanty, Lalit M. Pant Bhabha Atomic Research Centre, Trombay, Mumbai 400085, India Animesh ChatterjeeAC;HB, Sandhya Choubey, Raj Gandhi, Anushree GhoshAG;HB, Deepak TiwariHB Harish Chandra Research Institute, Jhunsi, Allahabad 211019, India Ali AjmiHB, S. Uma Sankar Indian Institute of Technology Bombay, Powai, Mumbai 400076, India Prafulla Behera, Aleena Chacko, Sadiq Jafer, James Libby, K. RaveendrababuHB, K. R. Rebin Indian Institute of Technology Madras, Chennai 600036, India D. Indumathi, K. MeghnaHB, S. M. LakshmiHB, M. V. N. Murthy, Sumanta PalSP;HB, G. RajasekaranGR, Nita Sinha Institute of Mathematical Sciences, Taramani, Chennai 600113, India Sanjib Kumar Agarwalla, Amina KhatunHB Institute of Physics, Sachivalaya Marg, Bhubaneswar 751005, India Poonam Mehta Jawaharlal Nehru University, New Delhi 110067, India Vipin Bhatnagar, R. Kanishka, A. Kumar, J. S. Shahi, J. B. Singh Panjab University, Chandigarh 160014, India Monojit GhoshMG, Pomita GhoshalPG, Srubabati Goswami, Chandan GuptaHB, Sushant RautSR Physical Research Laboratory, Navrangpura, Ahmedabad 380009, India Sudeb Bhattacharya, Suvendu Bose, Ambar Ghosal, Abhik JashHB, Kamalesh Kar, Debasish Majumdar, Nayana Majumdar, Supratik Mukhopadhyay, Satyajit Saha Saha Institute of Nuclear Physics, Bidhannagar, Kolkata 700064, India B. -
MINOS+: Running the MINOS Detectors in the Numi-Nova Beam
MINOS+: Running the MINOS Detectors in the Numi-NOvA Beam (FNAL P-1016) Presented by Alexander Radovic of University College London on behalf of the MINOS Collaboration. The Proposal: The Physics Reach: By continuing to the run the MINOS detectors during the NOvA Era Not only could MINOS+ augment the sin22ϴ and Δm2 we would hope to not only help NOvA improve on its measurement measurements of NOvA, it could also represent an opportunity of the oscillation parameters but also to probe new and interesting to probe some interesting areas of new physics. Such as: areas of physics, as well as improve our understanding of the neutrino beam flux. The Study of High Energy Neutrinos. Until now most neutrino oscillation experiments have focused on the lower The diagram on the right energies where the PMNS scenario tells us oscillations will shows the approximate occur. The MINOS detectors however would see the high energy regime that the MINOS energy tail of the NOvA beam, allowing for investigation MINOS detectors will be beyond the PMNS model of oscillations. sensitive to. Clearly very different to the spectrum The Search for seen at the NOvA Sterile Neutrinos. detectors it would give a NOvA The MINOS detectors window into a completely will see a large νμ flux different physical domain. from the NOvA beam which is perfect for With the MINOS detectors searching for a sterile we have a unique neutrino with opportunity to secure 2 2 2 m 4-m 3=O(1eV ) as Fermilab's position as a it would cause the world leader in Neutrino disappearance of research. -
Upgrade of the Minos+ Experiment Data Acquisition for the High Energy Numi Beam Run
FERMILAB-CONF-14-503-ND (accepted) Upgrade of the Minos+ Experiment Data Acquisition for the High Energy NuMI Beam Run William Badgett, Steve R. Hahn, Donatella Torretta, Jerry Meier, Jeffrey Gunderson, Denise Osterholm, David Saranen Abstract–The Minos+ experiment is an extension of the Minos Minos was designed a number of years before data taking experiment at a higher energy and more intense neutrino beam, commenced; by dint of technical progress, some of the with the data collection having begun in the fall of 2013. The electronics technology involved has become obsolete. The neutrino beam is provided by the Neutrinos from the Main Minos+ experiment was approved to extend the Minos data set Injector (NuMI) beam-line at Fermi National Accelerator Laboratory (Fermilab). The detector apparatus consists of two in the Noνa [2] NuMI beam era [3] with a higher energy and main detectors, one underground at Fermilab and the other in more intense neutrino beam. Both improved beam features Soudan, Minnesota with the purpose of studying neutrino result in higher signal occupancies in the Minos detector, and oscillations at a base line of 735 km. The original data especially so at the near detector located at Fermilab. The acquisition system has been running for several years collecting near detector is situated at 371 meters from the decay pipe, data from NuMI, but with the extended run from 2013, parts of while the far detector is 735 km away. At the peak beam the system needed to be replaced due to obsolescence, reliability problems, and data throughput limitations. Specifically, we have intensities of the high-energy run, we expect twenty neutrino replaced the front-end readout controllers, event builder, and interactions at the near detector per spill of ten micro-seconds data acquisition computing and trigger processing farms with duration at the near detector, compared to a maximum of three modern, modular and reliable devices with few single points of in the run ending in 2011.