First Direct Observation of the Tau Neutrino
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Decays of the Tau Lepton*
SLAC - 292 UC - 34D (E) DECAYS OF THE TAU LEPTON* Patricia R. Burchat Stanford Linear Accelerator Center Stanford University Stanford, California 94305 February 1986 Prepared for the Department of Energy under contract number DE-AC03-76SF00515 Printed in the United States of America. Available from the National Techni- cal Information Service, U.S. Department of Commerce, 5285 Port Royal Road, Springfield, Virginia 22161. Price: Printed Copy A07, Microfiche AOl. JC Ph.D. Dissertation. Abstract Previous measurements of the branching fractions of the tau lepton result in a discrepancy between the inclusive branching fraction and the sum of the exclusive branching fractions to final states containing one charged particle. The sum of the exclusive branching fractions is significantly smaller than the inclusive branching fraction. In this analysis, the branching fractions for all the major decay modes are measured simultaneously with the sum of the branching fractions constrained to be one. The branching fractions are measured using an unbiased sample of tau decays, with little background, selected from 207 pb-l of data accumulated with the Mark II detector at the PEP e+e- storage ring. The sample is selected using the decay products of one member of the r+~- pair produced in e+e- annihilation to identify the event and then including the opposite member of the pair in the sample. The sample is divided into subgroups according to charged and neutral particle multiplicity, and charged particle identification. The branching fractions are simultaneously measured using an unfold technique and a maximum likelihood fit. The results of this analysis indicate that the discrepancy found in previous experiments is possibly due to two sources. -
Probing Light Gauge Bosons in Tau Neutrino Experiments
Probing Light Gauge Bosons in Tau Neutrino Experiments Felix Kling∗ SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025, USA The tau neutrino is probably the least studied particle in the SM, with only a handful of interaction events being identified so far. This can in part be attributed to their small production rate in the SM, which occurs mainly through Ds meson decay. However, this also makes the tau neutrino flux measurement an interesting laboratory for additional new physics production modes. In this study, we investigate the possibility of tau neutrino production in the decay of light vector bosons. We consider four scenarios of anomaly-free U(1) gauge groups corresponding to the B−L, B−Lµ−2Lτ , B − Le − 2Lτ and B − 3Lτ numbers, analyze current constraints on their parameter spaces and explore the sensitivity of DONuT and as well as the future emulsion detector experiments FASERν, SND@LHC and SND@SHiP. We find that these experiments provide the leading direct constraints in parts of the parameter space, especially when the vector boson's mass is close to the mass of the ! meson. I. INTRODUCTION other neutrino flavors. This small SM production rate makes the tau neutrino flux measurement an interesting The standard model (SM) consist of 17 particles, out laboratory for additional beyond the SM (BSM) produc- tion modes. of which the tau neutrino ντ is the least experimentally constrained one. To detect the rare tau neutrino interac- One example of such new physics are light vector tions, an intense neutrino beam with a sufficiently large bosons V associated with additional gauge groups. -
J = Τ MASS Page 1
Citation: P.A. Zyla et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2020, 083C01 (2020) J 1 τ = 2 + + τ discovery paper was PERL 75. e e− → τ τ− cross-section threshold behavior and magnitude are consistent with pointlike spin- 1/2 Dirac particle. BRANDELIK 78 ruled out pointlike spin-0 or spin-1 particle. FELDMAN 78 ruled out J = 3/2. KIRKBY 79 also ruled out J=integer, J = 3/2. τ MASS VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 1776..86 0..12 OUR AVERAGE ± +0.10 1776.91 0.12 1171 1 ABLIKIM 14D BES3 23.3 pb 1, Eee = ± 0.13 − cm − 3.54–3.60 GeV 1776.68 0.12 0.41 682k 2 AUBERT 09AK BABR 423 fb 1, Eee =10.6 GeV ± ± − cm 1776.81+0.25 0.15 81 ANASHIN 07 KEDR 6.7 pb 1, Eee = 0.23 ± − cm − 3.54–3.78 GeV 1776.61 0.13 0.35 2 BELOUS 07 BELL 414 fb 1 Eee =10.6 GeV ± ± − cm 1775.1 1.6 1.0 13.3k 3 ABBIENDI 00A OPAL 1990–1995 LEP runs ± ± 1778.2 0.8 1.2 ANASTASSOV 97 CLEO Eee = 10.6 GeV ± ± cm . +0.18 +0.25 4 Eee . 1776 96 0.21 0.17 65 BAI 96 BES cm= 3 54–3 57 GeV − − 1776.3 2.4 1.4 11k 5 ALBRECHT 92M ARG Eee = 9.4–10.6 GeV ± ± cm +3 6 Eee 1783 4 692 BACINO 78B DLCO cm= 3.1–7.4 GeV − We do not use the following data for averages, fits, limits, etc. -
Tau (Or No) Leptons in Top Quark Decays at Hadron Colliders
Tau (or no) leptons in top quark decays at hadron colliders Michele Gallinaro for the CDF, D0, ATLAS, and CMS collaborations Laborat´oriode Instrumenta¸c˜aoe F´ısicaExperimental de Part´ıculas LIP Lisbon, Portugal DOI: http://dx.doi.org/10.3204/DESY-PROC-2014-02/12 Measurements in the final states with taus or with no-leptons are among the most chal- lenging as they are those with the smallest signal-to-background ratio. However, these final states are of particular interest as they can be important probes of new physics. Tau identification techniques and cross section measurements in top quark decays in these final states are discussed. The results, limited by systematical uncertainties, are consistent with standard model predictions, and are used to set stringent limits on new physics searches. The large data samples available at the Fermilab and at the Large Hadron Collider may help further improving the measurements. 1 Introduction Many years after its discovery [1, 2], the top quark still plays a fundamental role in the program of particle physics. The study of its properties has been extensively carried out in high energy hadron collisions. The production cross section has been measured in many different final states. Deviation of the cross section from the predicted standard model (SM) value may indicate new physics processes. Top quarks are predominantly produced in pairs, and in each top quark pair event, there are two W bosons and two bottom quarks. From the experimental point of view, top quark pair events are classified according to the decay mode of the two W bosons: the all-hadronic final state, in which both W bosons decay into quarks, the “lepton+jet” final state, in which one W decays leptonically and the other to quarks, and the dilepton final state, in which both W bosons decay leptonically. -
Search for Rare Multi-Pion Decays of the Tau Lepton Using the Babar Detector
SEARCH FOR RARE MULTI-PION DECAYS OF THE TAU LEPTON USING THE BABAR DETECTOR DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Ruben Ter-Antonyan, M.S. * * * * * The Ohio State University 2006 Dissertation Committee: Approved by Richard D. Kass, Adviser Klaus Honscheid Adviser Michael A. Lisa Physics Graduate Program Junko Shigemitsu Ralph von Frese ABSTRACT A search for the decay of the τ lepton to rare multi-pion final states is performed + using the BABAR detector at the PEP-II asymmetric-energy e e− collider. The anal- 1 ysis uses 232 fb− of data at center-of-mass energies on or near the Υ(4S) resonance. + 0 In the search for the τ − 3π−2π 2π ν decay, we observe 10 events with an ex- ! τ +2:0 pected background of 6:5 1:4 events. In the absence of a signal, we calculate the − + 0 6 decay branching ratio upper limit (τ − 3π−2π 2π ν ) < 3:4 10− at the 90 % B ! τ × confidence level. This is more than a factor of 30 improvement over the previously established limit. In addition, we search for the exclusive decay mode τ − 2!π−ν ! τ + 0 +1:0 with the further decay of ! π−π π . We observe 1 event, expecting 0.4 0:4 back- ! − 7 ground events, and calculate the upper limit (τ − 2!π−ν ) < 5:4 10− at the B ! τ × 90 % confidence level. This is the first upper limit for this mode. -
Dstau: Study of Tau Neutrino Production with 400 Gev Protons from the CERN-SPS
Prepared for submission to JHEP DsTau: Study of tau neutrino production with 400 GeV protons from the CERN-SPS Shigeki Aoki,a Akitaka Ariga,b;1 Tomoko Ariga,b;c Sergey Dmitrievsky,d Elena Firu,e Dean Forshaw,b Tsutomu Fukuda,f Yuri Gornushkin,d Ali Murat Guler,g Maria Haiduc,e Koichi Kodama,h Masahiro Komatsu,f Muhtesem Akif Korkmaz,g Umut Kose,i Madalina Miloi,e Antonio Miucci,b Motoaki Miyanishi,f Mitsuhiro Nakamura,f Toshiyuki Nakano,f Alina Neagu,e Hiroki Rokujo,f Osamu Sato,f Elizaveta Sitnikova,d Yosuke Suzuki,f Tomoki Takao,f Svetlana Vasina,d Mykhailo Vladymyrov,b Thomas Weston,b Junya Yoshida,j Masahiro Yoshimoto.k The DsTau Collaboration aKobe University, Kobe, Japan bAlbert Einstein Center for Fundamental Physics, Laboratory for High Energy Physics, University of Bern, Bern, Switzerland cKyushu University, Fukuoka, Japan dJoint Institute for Nuclear Research, Dubna, Russia eInstitute of Space Science, Bucharest, Romania f Nagoya University, Nagoya, Japan gMiddle East Technical University, Ankara, Turkey hAichi University of Education, Kariya, Japan iCERN, Geneva, Switzerland jAdvanced Science Research Center, Japan Atomic Energy Agency, Tokai, Japan kGifu University, Gifu, Japan E-mail: [email protected] Abstract: In the DsTau experiment at the CERN SPS, an independent and direct way to measure tau neutrino production following high energy proton interactions was proposed. As the main source of tau neutrinos is a decay of Ds mesons, produced in proton-nucleus arXiv:1906.03487v1 [hep-ex] 8 Jun 2019 interactions, the project aims at measuring a differential cross section of this reaction. The experimental method is based on a use of high resolution emulsion detectors for effective registration of events with short lived particle decays. -
Detection of the Tau-Neutrino at The
DETECTION OF THE TAIPNEIITRINO AT me LI·IC* Klaus Winter CERN. Geneva. Switzerland I. Introduction Following the discovery of the tau-lepton in e+e` collisions by M. Perl and collabo rators [1 ], all evidence today favours the hypothesis that it is a sequential heavy lepton belonging to a third lepton Family [2]. From measurements of the forward-bacl< ward angular asymmetry of tau produced in e+e` annihilations [3], [4] e+e* +* ft a value of the axial-vector neutral current coupling constant of ga = — 0.—l5 1 0.05 was deduced in agreement with ga = -1 /2 for the assignment of lel’t—handed tau leptons as the "down" state (I3 = -1 /2) of a weak isospin doublet. Hence, the most natural assignment of the "up" state (I3 = +1/2) would be to a neutrino with the same lepton flavour. the tau-neutrino. Further indirect evidence about the tau—neutrino can be obtained from leptonic tau decays [4]. e.g. 1:- Q u_v,,X. The muon energy spectrum has the familiar [2] Michel shape suggesting that the par ticle X is a spin l /2 particle. Its mass has been constrained to less than 35 MeV by analysing semi-leptonic tau—deca)s with multipion final states [5]. Hence, the particle Xmay be a neutrino. Is it a sequential neutrino, with a flavour property which distin guishes it from the electron- and the muon-neutrino? The possibility of a complete identity with we or uu can indeed be excluded. Searches for charged current neutrino reactions which produce a tau-lepton UN ·=* T_X have given negative results. -
Neutrino Physics
0 Neutrino Physics Zhi-zhong Xing ★ Neutrino’s history & lepton families (IHEP, Beijing) ★ Dirac & Majorana neutrino masses ★ Lepton flavor mixing & CP violation ★ Neutrino oscillation phenomenology ★ Seesaw & leptogenesis mechanisms ★ Extreme corners in the neutrino sky Lecture A @ the 2nd Asia-Europe-Pacific School of HEP, 11/2014, Puri, India Neutrinos everywhere 1 SM Properties: charge = 0 spin = ½ mass = 0 Big Bang speed = c neutrinos Galaxy Human Supernova Sun Earth Reactor Accelerator Neutrinos: witness and participant 1 in the evolution of the Universe 3 2 < 1% Some open questions 3 . the absolute mass scale? . the mass hierarchy? . the flavor desert? . leptonic CP violation? . the Majorana nature? . How many species? . cosmic background? . supernova & stellar ’s? . UHE cosmic ’s? . warm dark matter? . matter-antimatter asymmetry… Lecture A1 ★ Neutrinos from new physics ★ Interactions and discoveries ★ Flavors / families of leptons Beta decays in 1930 5 2-body Energy crisis = New physics ? decays J. Chadwick 1914/C. Ellis 1920-1927 What to do? Two ways out? 6 . giving up sth . adding in sth Niels Bohr Wolfgang Pauli (1930) Pauli put forward this idea in a letter instead of a paper….. Solvay 1933 7 Pauli gave a talk on his neutrino proposal in this congress. Fermi’s theory 8 Enrico Fermi assumed a new force for I will be remembered decay by combining 3 new concepts: for this paper. ------ Fermi in Italian ★ Pauli’s idea: neutrinos Alps, Christmas 1933 ★ Dirac’s idea: creation of particles ★ Heisenberg’s idea: isospin symmetry Fermi’s paper 9 This is Fermi’s best theoretical work! ---- C.N. Yang Published first in this journal and later in Z. -
Masses of the Sub-Nuclear Particles Fit Into One Equation
Masses of the Sub-Nuclear Particles Theodore M. Lach The masses of the quarks and leptons are for the most part a mystery to particle physicists. Currently there seems to be no correlation between the masses of the elementary particles. This paper is an attempt to formulate a theory that would begin to explain the relationship between the sub-nuclear particle masses. A key premise of the Standard Model is that there are 3 and only 3 generations of quarks and leptons. The currently accepted masses of these elementary particles are: (1) Table 1. Generation # 1 Generation # 2 Generation # 3 Up quark = 3 MeV, (1-5) Charmed quark = 1.25+0.1 GeV Top quark = 175 +5 GeV Down quark = 6 MeV Strange quark = 100 MeV Bottom quark = 4.2 GeV (3-9 MeV) (75-170 MeV) + 0.2 GeV Electron = 0.5109989MeV Muon = 105.6583 MeV Tau = 1777.1 MeV The neutrino masses in the standard model are still a hotly debated issue, yet arXiv:nucl-th/0008026 14 Aug 2000 most current references put the upper bound of the three neutrinos at: Table 2. Electron neutrino = 10 ev (5 – 17 ev) Muon neutrino = 270 KeV (200 – 270 KeV) Tau neutrino = 31 MeV (20 – 35 MeV) In an attempt to determine why the quark masses predicted in the CBM (2), Checker Board Model of the nucleus, do not fit into the standard model, I will deviate from the S.M. and assume that my quark masses in table 3 are correct and that there are more than 3 generations. -
The Tau and Beyond: Future Research on Heavy Leptons*
SLAC-PUB-4819 January 1988 Pm) THE TAU AND BEYOND: FUTURE RESEARCH ON HEAVY LEPTONS* MARTIN L. PERL Stanford Linear Accelerator Center Stanford University, Stanford, California 94309 . ABSTRACT: This paper outlines directions for future experimental research on the tau and tau neutrino. Present limits on the existence of heavier charged leptons are re- viewed, with emphasis on the close-mass lepton pair con- cept. *Work supported by the Department of Energy, contract DE-AC03-76SF00515. Presented at the 8th International Conference on Physics in Collision, Capri, Italy, October 19-21, 1988. Table of Contents I. Introduction II. The Tau A. The Decay Mode Problem B. Better Measurements of Conventional Properties C. Tau Lepton Number Conservation D. Deviations From a Dirac Point Particle E. The Concept of Lepton-Specific Forces and the Tau III. The Tau Neutrino A. Tau Neutrino Mass B. Tau Neutrino Mixing C. Interactions of the Tau Neutrino D. Variations on the Tau Neutrino IV. Limits on the Existence of Heavier Charged Leptons A. Present Limits B. Future Searches for Charged Leptons I. Introduction In 1981, at the first Physics In Collision Conference, I reviewed the status of the tau and of the search for heavier leptons. Now, seven years later, I have the pleasure of presenting another such review. Those seven years demonstrate the perversity of nature, or more precisely, demonstrate the obstinacy of nature with respect to the desires and expectations of the physicist. By 1981 the tau was established and the particle physicist looked forward to the discovery of more and heavier leptons. Two new electron-positron colliders PETRA and PEP were in operation, and the CERN pp collider was under construction. -
Physics with Tau Lepton Final States in ATLAS
EPJ Web of Conferences 49, 18022 (2013) DOI: 10.1051/epjconf/ 20134918022 C Owned by the authors, published by EDP Sciences, 2013 Physics with Tau Lepton Final States in ATLAS Almut M. Pingel1,a, on behalf of the ATLAS Collaboration 1Niels Bohr Institute, University of Copenhagen Abstract. The ATLAS detector records collisions from two high-energetic proton beams circulating in the LHC. An integral part of the ATLAS physics program are analyses with tau leptons in the final state. Here an overview is given over the studies done in ATLAS with hadronically-decaying final state tau leptons: Standard Model cross-section measurements of Z ⌧⌧, W ⌧⌫ and tt¯ bbe¯ /µ⌫ ⌧ ⌫; ⌧ polarization measurements ! ! ! had in W ⌧⌫ decays; Higgs searches and various searches for physics beyond the Standard Model. ! 1 Introduction 2 Standard Model cross-section measurements The ATLAS [1] physics program covers a wide range of analyses with tau leptons in the final state, which are The SM processes W ⌧⌫ and Z ⌧⌧ are backgrounds ! ! important both to test the Standard Model (SM) and in in many studies with final state tau leptons, in particular in searches for new physics. In 2010 and 2011, the LHC [2] searches for the Higgs boson. It is therefore important to was operated at a center-of-mass energy of ps = 7 TeV, study and measure the cross-sections precisely. Further- and at ps = 8 TeV in 2012. Physics searches presented more, deviations from predicted SM cross-sections are an 1 here are based on the full 2011 dataset of 4.7 fb− if not indicator for new physics processes. -
Discoverers of the Neutrino and Tau Recognised
RESEARCH I NEWS Discoverers of the Neutrino the turn of two of the six leptons of today's and Tau Recognised particle physics, the electron-neutrino ve and the T lepton, tau, to acquire 'Nobelity'. Particles that Acq ui red 'hlobei ity' K V L Sarma Frederick Reines (University of California, Irvine), now 77,with Clyde L Cowan Jr. (who The 1995 Nobel Prize in Physics is shared by died in 1974) reported the first direct evidence the American physicists Frederick J Reines of the existence of the 'neutrino' in 1956. The and Martin L Perl for their pioneering experi neutrino is a tiny neutral particle hypoth mental contributions to 'lepton' physics. Lep esized by Wolfgang Pauli Jr. in 1930. Twenty tons, such as the electron, do not feel the five years later and with the invention of the nuclear force but only the electromagnetic nuclear reactor it was possible to verify its and the weak beta decay force. This year it is existence. This year's Nobel award in Physics is in recognition belong. A summary of the discoveries made in the of two landmark experiments in elementary par world of leptons is given in the table below. The ticle physics. One provided the confirmation of the third generation has now started getting Nobel neutrino, as envisaged by Pauli more than two prizes. It should be noted that v T still needs to be decades earlier. The second discovered the heavy identified experimentally land hence the question charged lepton "t which heralded the third, and marks in the last row of the table!.