Searching for Muon to Electron Conversion: the Mu2e Experiment at Fermilab
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The Mu3e Experiment
Nuclear Physics B Proceedings Supplement Nuclear Physics B Proceedings Supplement 00 (2013) 1–6 The Mu3e Experiment Niklaus Berger for the Mu3e Collaboration Physikalisches Institut, Heidelberg University Abstract The Mu3e experiment is designed to search for charged lepton flavour violation in the process µ+ ! e+e−e+ with a branching ratio sensitivity of 10−16. This requires a detector capable of coping with rates of up to 2 · 109 muons=s + + − + whilst being able to reduce backgrounds from accidental coincidences and the process µ ! e e e ν¯µνe to below the 10−16 level. The use of 50 µm thin high-voltage monolithic active pixel sensors in conjunction with an innovative tracking concept provide the momentum and position resolution necessary, whilst the timing resolution is provided by a combination of scintillating fibres and tiles. The recently approved Mu3e experiment will be located at the Paul Scherrer Institute in Switzerland and is currently preparing for detector construction. Keywords: Charged lepton flavour violation, Pixel Sensors, Muon Beams 1. Motivation many models. In the case of muons, the processes un- der study are the decay µ+ ! e+γ, the conversion of The discovery of neutrino oscillations has revealed a muon to an electron in the field of a nucleus and the that lepton flavour is not a conserved quantum number. process µ+ ! e+e−e+; an overview of the experimental Despite of a long history of searches (see e.g. [1, 2, 3] status for these three processes is given in Table 1. for reviews), no flavour violation has ever been observed The Mu3e experiment [9] is designed to search for in the charged lepton sector; these non-observations µ+ ! e+e−e+ with a branching ratio sensitivity of being one of the observational pillars on which the < 10−16, an improvement by four orders of magnitude Standard Model (SM) of particle physics is built. -
Muon Decay 1
Muon Decay 1 LIFETIME OF THE MUON Introduction Muons are unstable particles; otherwise, they are rather like electrons but with much higher masses, approximately 105 MeV. Radioactive nuclear decays do not release enough energy to produce them; however, they are readily available in the laboratory as the dominant component of the cosmic ray flux at the earth’s surface. There are two types of muons, with opposite charge, and they decay into electrons or positrons and two neutrinos according to the rules + + µ → e νe ν¯µ − − µ → e ν¯e νµ . The muon decay is a radioactiveprocess which follows the usual exponential law for the probability of survival for a given time t. Be sure that you understand the basis for this law. The goal of the experiment is to measure the muon lifetime which is roughly 2 µs. With care you can make the measurement with an accuracy of a few percent or better. In order to achieve this goal in a conceptually simple way, we look only at those muons that happen to come to rest inside our detector. That is, we first capture a muon and then measure the elapsed time until it decays. Muons are rather penetrating particles, they can easily go through meters of concrete. Nevertheless, a small fraction of the muons will be slowed down and stopped in the detector. As shown in Figure 1, the apparatus consists of two types of detectors. There is a tank filled with liquid scintillator (a big metal box) viewed by two photomultiplier tubes (Left and Right) and two plastic scintillation counters (flat panels wrapped in black tape), each viewed by a photomul- tiplier tube (Top and Bottom). -
The Muon Guys on the Hunt for New Physics
THE MUON GUYS ON THE HUNT FOR NEW PHYSICS BY Andrea MustaIN PHOTOGRAPHY BY REIDAR HAHN, FERMILAB 10 of mysterious equipment in a workroom at AMID A sprawL Fermi National Accelerator Laboratory, Gueorgui Velev and Alexander Makarov leaned over an elegant metal box the size of a single file cabinet. Suffused by a warm halo of late-afternoon sunlight, the two men, a physicist and an engineer, had the look of modern-day priests of industry gently handling a beloved reliquary. Velev lifted the box top, revealing a thin slice of dark-gray ferrite—a ceramic compound used in powerful magnets. Although the ferrite was wired up like an intensive-care patient, for the moment it felt cool and deliciously smooth to the touch. Velev and Makarov have been testing ferrites like this one for almost a year now, send- ing powerful currents through the compound, pushing the material to its limits. Far from being a relic of something dead, the ferrite is a symbol of resurrection for an experiment that could star in its own soap opera. Attempts to carry out this experiment have died two deaths on two continents over the course of two decades. Velev and Makarov, along with a host of collaborators, are once again bringing it to life. The experiment’s newest name, in its incarnation at Fermilab, is Mu2e (pronounced Mew to E), which stands for muon-to-electron conversion; and it is a testament to the strength of the science behind this experiment that physicists are still fighting to do it. Scientists plan to break ground at Fermilab in Batavia, Illinois, in 2013 and begin taking data four years later. -
Searching for Muon to Electron Conversion: the Design of the Mu2e Experiment
Searching for Muon to electron conversion: The design of the Mu2e experiment Richie Bonventre Physics 290e Lawrence Berkeley National Lab The physics of Mu2e • Mu2e will search for neutrinoless conversion of a muon to an electron in a nuclear environment: µ−N → e−N • This would violate charged lepton flavor, something that has never been seen before • Any detection of charged lepton flavor violation would be an unambiguous sign of new physics! (SM contribution is < 10−50) 1/46 Charged Lepton Flavor Violation • Neutrino oscillation shows that Lepton Flavor is NOT a fundamental symmetry. No reason new physics should conserve it • Many models of new physics predict contributions to CLFV: 2/46 History Mu2e goal is a 104 improvement! 3/46 Types of CLFV measurements Process Current Limit Next Generation exp. τ → µη BR < 6.5 E-8 10−9 - 10−10 (Belle II, LHCb) τ → µγ BR < 6.8 E-8 τ → µµµ BR < 3.2 E-8 τ → eee BR < 3.6 E-8 KL →eµ BR < 4.7 E-12 K+ → π+e−µ+ BR < 1.3 E-11 B0 →eµ BR < 7.8 E-8 B+ →K+eµ BR < 9.1 E-8 µ+ →e+γ BR < 4.2 E-13 10−14 (MEG) µ+ →e+e+e− BR < 1.0 E-12 10−16 (PSI) − − −17 µ N→e N Rµe < 7.0 E-13 10 (Mu2e, COMET) 4/46 How to search for CLFV • τ seems easiest at first • Larger mass reduces GIM suppression, most models predict larger BF • Larger mass means more possible decay modes • But lifetime is very short • Much easier to produce a lot of muons (which is good because we need 1018!) p + p/n → n + p/n + π π → µ + ν 5/46 Muon CLFV processes: µ → eγ, µ → eee, µN→ eN • µ → eγ • Signal is back-to-back monoenergetic electron, gamma at 52.8 -
Muon Neutrino Mass Without Oscillations
The Distant Possibility of Using a High-Luminosity Muon Source to Measure the Mass of the Neutrino Independent of Flavor Oscillations By John Michael Williams [email protected] Markanix Co. P. O. Box 2697 Redwood City, CA 94064 2001 February 19 (v. 1.02) Abstract: Short-baseline calculations reveal that if the neutrino were massive, it would show a beautifully structured spectrum in the energy difference between storage ring and detector; however, this spectrum seems beyond current experimental reach. An interval-timing paradigm would not seem feasible in a short-baseline experiment; however, interval timing on an Earth-Moon long baseline experiment might be able to improve current upper limits on the neutrino mass. Introduction After the Kamiokande and IMB proton-decay detectors unexpectedly recorded neutrinos (probably electron antineutrinos) arriving from the 1987A supernova, a plethora of papers issued on how to use this happy event to estimate the mass of the neutrino. Many of the estimates based on these data put an upper limit on the mass of the electron neutrino of perhaps 10 eV c2 [1]. When Super-Kamiokande and other instruments confirmed the apparent deficit in electron neutrinos from the Sun, and when a deficit in atmospheric muon- neutrinos likewise was observed, this prompted the extension of the kaon-oscillation theory to neutrinos, culminating in a flavor-oscillation theory based by analogy on the CKM quark mixing matrix. The oscillation theory was sensitive enough to provide evidence of a neutrino mass, even given the low statistics available at the largest instruments. J. M. Williams Neutrino Mass Without Oscillations (2001-02-19) 2 However, there is reason to doubt that the CKM analysis validly can be applied physically over the long, nonvirtual propagation distances of neutrinos [2]. -
Theory Challenges and Opportunities of Mu2e-II: Letter of Interest for Snowmass 2021
Theory challenges and opportunities of Mu2e-II: Letter of Interest for Snowmass 2021 Robert H. Bernstein,1 Leo Borrel,2 Lorenzo Calibbi,3, ∗ Andrzej Czarnecki,4 Sacha Davidson,5 Bertrand Echenard,2 Julian Heeck,6, y David G. Hitlin,2 William Marciano,7 Sophie C. Middleton,2 Vitaly S. Pronskikh,1 and Robert Szafron8 1Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA 2California Institute of Technology, Pasadena, California 91125, USA 3School of Physics, Nankai University, Tianjin 300071, China 4Department of Physics, University of Alberta, Edmonton, Alberta T6G 2E1, Canada 5LUPM, CNRS, Universit´eMontpellier, Place Eugene Bataillon, F-34095 Montpellier, Cedex 5, France 6Department of Physics, University of Virginia, Charlottesville, Virginia 22904, USA 7Department of Physics, Brookhaven National Laboratory, Upton, New York 11973, USA 8Theoretical Physics Department, CERN, 1211 Geneva 23, Switzerland Searches for lepton flavor violation are extremely sensitive to physics beyond the Standard Model. Several experiments are going to probe uncharted parameter space in the near future; notably, the Mu2e experiment is aiming to improve sensitivity to µ− ! e− conversion in nuclei by several orders of magnitude over existing limits. Mu2e-II marks a potential upgrade of Mu2e with another order-of-magnitude increase in sensitivity. This remarkable reach will make Mu2e(-II) an important experiment to probe new physics, not only via µ− ! e− conversion, but potentially also via µ− ! e+ conversion or µ− ! e−X decays involving a light new boson X. Theory challenges of this project include comparing the sensitivity of different experiments to a given model, evaluating possible stopping targets to maximize complementarity, and understanding the unavoidable muon-decay-in- orbit background at this unprecedented precision. -
Muons: Particles of the Moment
FEATURES Measurements of the anomalous magnetic moment of the muon provide strong hints that the Standard Model of particle physics might be incomplete Muons: particles of the moment David W Hertzog WHEN asked what the most important strange, bottom and top; and six leptons, issue in particle physics is today, my ABORATORY namely the electron, muon and tau- colleagues offer three burning ques- L lepton plus their associated neutrinos. ATIONAL tions: What is the origin of mass? Why N A different set of particles is respon- is the universe made of matter and not sible for the interactions between these equal parts of matter and antimatter? ROOKHAVEN matter particles in the model. The elec- And is there any physics beyond the B tromagnetic interaction that binds elec- Standard Model? trons to nuclei results from the exchange The first question is being addressed of photons, whereas the strong force by a feverish quest to find the Higgs that binds quarks together inside neut- boson, which is believed to be respon- rons, protons and other hadrons is car- sible for the mass of fundamental par- ried by particles called gluons. The ticles. The Tevatron at Fermilab, which third force in the Standard Model – the is currently running, or the Large Had- weak nuclear interaction, which is re- ron Collider at CERN, which is due sponsible for radioactive decay – is car- to start experiments in 2007, should OWMAN ried by the W and Z bosons. B IPP eventually provide the answer to this R Physicists love the Standard Model, question by detecting the Higgs and but they do not like it. -
The Mu2e Experiment at Fermilab⇤
NuFact15 - Rio de Janeiro, Brazil - August 2015 The Mu2e Experiment at Fermilab⇤ 1, 2, Kevin R. Lynch † , (The Fermilab Mu2e Collaboration) ‡ 1Department of Earth and Physical Sciences, York College, City University of New York, 94-20 Guy R. Brewer Blvd, Jamaica, NY 11451 USA 2The Graduate Center, City University of New York, 365 Fifth Avenue New York, NY 10016 USA (Dated: April 18, 2016) 449 NuFact15 - Rio de Janeiro, Brazil - August 2015 Abstract The Mu2e Experiment at Fermilab will search for the coherent, neutrinoless conversion of a muon to an electron in the field of an atomic nucleus. Such charged lepton flavor violating events have never been observed, but are predicted to occur in many Beyond the Standard Model scenarios at rates accessible to our experiment. I outline the physics and key issues for the experiment, our progress on design and construction to date, and prospects for the future. INTRODUCTION The Mu2e e↵ort holds a prominent place in the near term future of the U.S. High Energy Physics program. In fact, the recent report of the Particle Physics Project Prioritization Panel (P5) - which advises the U.S. Government on HEP community priorities - advises completion of the Mu2e Experiment under all budget scenarios considered [1]. With a project baseline cost of $270 million, this involves a significant investment of available resources; why, then, this level of interest? Although charged lepton flavor violation (CLFV) has never been observed experimentally, we know that it must occur: neutrino flavor oscillations coupled with loops guarantees the existence of CLFV; see Figure 1. However, even with the most optimistic parameter values in the PMNS neutrino mixing matrix U, the Standard Model rate prediction is tiny 2 2 3↵ ∆m1k 54 Br(µ eγ)= Uµk⇤ Uek 2 < 10− . -
Arxiv:1512.01765V2 [Physics.Atom-Ph]
August12,2016 1:27 WSPCProceedings-9.75inx6.5in Antognini˙ICOLS˙3 page 1 1 Muonic atoms and the nuclear structure A. Antognini∗ for the CREMA collaboration Institute for Particle Physics, ETH, 8093 Zurich, Switzerland Laboratory for Particle Physics, Paul Scherrer Institute, 5232 Villigen-PSI, Switzerland ∗E-mail: [email protected] High-precision laser spectroscopy of atomic energy levels enables the measurement of nu- clear properties. Sensitivity to these properties is particularly enhanced in muonic atoms which are bound systems of a muon and a nucleus. Exemplary is the measurement of the proton charge radius from muonic hydrogen performed by the CREMA collaboration which resulted in an order of magnitude more precise charge radius as extracted from other methods but at a variance of 7 standard deviations. Here, we summarize the role of muonic atoms for the extraction of nuclear charge radii, we present the status of the so called “proton charge radius puzzle”, and we sketch how muonic atoms can be used to infer also the magnetic nuclear radii, demonstrating again an interesting interplay between atomic and particle/nuclear physics. Keywords: Proton radius; Muon; Laser spectroscopy, Muonic atoms; Charge and mag- netic radii; Hydrogen; Electron-proton scattering; Hyperfine splitting; Nuclear models. 1. What atomic physics can do for nuclear physics The theory of the energy levels for few electrons systems, which is based on bound- state QED, has an exceptional predictive power that can be systematically improved due to the perturbative nature of the theory itself [1, 2]. On the other side, laser spectroscopy yields spacing between energy levels in these atomic systems so pre- cisely, that even tiny effects related with the nuclear structure already influence several significant digits of these measurements. -
Status of the Mu2e Experiment at Fermilab
EPJ Web of Conferences 234, 01010 (2020) https://doi.org/10.1051/epjconf/202023401010 FCCP2019 Status of the Mu2e experiment at Fermilab Stefano Miscetti1;a on behalf of the Mu2e Collaboration 1Laboratori Nazionali di Frascati dell’INFN, Via Enrico Fermi 40, 00044, Frascati, Italy Abstract. The Mu2e experiment aims to improve, by four orders of magnitude, current sensitivity in the search for the charged-lepton flavor violating (cLFV) neutrino-less conversion of a negative muon into an electron. The conversion process will be identified by a distinctive signature of a mono-energetic electron with energy slightly below the muon rest mass. In the Standard Model this process has a negligible rate. However, in many Beyond the Standard Model scenarios its rate is within the reach of Mu2e sensitivity. In this paper, we explain the Mu2e design guidelines and summarize the status of the experiment. 1 Introduction A solid international program continues nowadays with the upgrade of MEG [7, 8], the proposed Mu3e search Since flavor violation has been established in quarks and at PSI [7, 9] as well as the searches for muon to electron neutrinos, it is natural to expect flavor violating processes conversion with Mu2e at Fermilab [10] and COMET at J- also among the charged leptons. Albeit in the Standard PARC [7, 11]. These experiments plan to extend the cur- Model (SM) there is not any global symmetry requiring rent sensitivity of one or more orders of magnitude pro- lepton flavor violation, when massive neutrinos are in- viding access to new physics mass scales in the 103 -104 troduced, the SM provides a mechanism for cLFV via GeV range, well beyond what can be directly probed at neutrino-mixing in loops. -
The Mu2e Experiment at Fermilab: a Search for Charged Lepton Flavor Violation
The Mu2e Experiment at Fermilab: a Search for Charged Lepton Flavor Violation James Miller, Boston University, R. Bernstein, FNAL, on behalf of the Mu2e Collaboration. A new experiment, Mu2e, is being developed at Fermilab to measure the ratio of the rate of the neutrinoless, coherent conversion of muons into electrons in the field of a nucleus, relative to the rate of ordinary muon capture on the nucleus, P oA(,Z N )e A (,Z N ) RPe PQoA(,Z N )P A (Z 1,)N Mu2e expects a four orders of magnitude improvement on the experimental uncertainty in this ratio, providing a stringent test of the SM with an energy scale on the order of thousands of TeV. The conversion process is an example of charged lepton flavor violation (cLFV), where muon and electron numbers change by -1 and 1, respectively. Until the discovery of neutrino oscillations, lepton numbers in each generation were strictly conserved in the Standard Model (SM) for any interaction. In a simple extension of the SM that includes neutrino oscillations, an extremely small rate of muon to electron conversion is predicted, far below any foreseeable experimental sensitivity. Therefore a non-vanishing signal would be a definite sign of new physics. In most of the proposed models of physics beyond the SM, cLFV is allowed. Better experimental limits on cLFV processes produce ever tighter limits on the available parameters in these models. Although the existence of lepton generations and conservation of lepton numbers plays a central role in the SM, there is no understanding of the underlying symmetry that causes it. -
Explaining Muon G − 2 Data in the Μνssm Arxiv:1912.04163V3 [Hep-Ph]
Explaining muon g 2 data in the µνSSM − Essodjolo Kpatcha∗a,b, Iñaki Lara†c, Daniel E. López-Fogliani‡d,e, Carlos Muñoz§a,b, and Natsumi Nagata¶f aDepartamento de Física Teórica, Universidad Autónoma de Madrid (UAM), Campus de Cantoblanco, 28049 Madrid, Spain bInstituto de Física Teórica (IFT) UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain cFaculty of Physics, University of Warsaw, Pasteura 5, 02-093 Warsaw, Poland dInstituto de Física de Buenos Aires UBA & CONICET, Departamento de Física, Facultad de Ciencia Exactas y Naturales, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina e Pontificia Universidad Católica Argentina, 1107 Buenos Aires, Argentina fDepartment of Physics, University of Tokyo, Tokyo 113-0033, Japan Abstract We analyze the anomalous magnetic moment of the muon g 2 in the µνSSM. − This R-parity violating model solves the µ problem reproducing simultaneously neu- trino data, only with the addition of right-handed neutrinos. In the framework of the µνSSM, light left muon-sneutrino and wino masses can be naturally obtained driven by neutrino physics. This produces an increase of the dominant chargino-sneutrino loop contribution to muon g 2, solving the gap between the theoretical computation − and the experimental data. To analyze the parameter space, we sample the µνSSM using a likelihood data-driven method, paying special attention to reproduce the cur- rent experimental data on neutrino and Higgs physics, as well as flavor observables such as B and µ decays. We then apply the constraints from LHC searches for events with multi-leptons + MET on the viable regions found. They can probe these regions through chargino-chargino, chargino-neutralino and neutralino-neutralino pair pro- duction.