Underground Neutrino Experiment Sets the Stage for Deep Discovery About Matter
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Ettore Majorana: Genius and Mystery
«ETTORE MAJORANA» FOUNDATION AND CENTRE FOR SCIENTIFIC CULTURE TO PAY A PERMANENT TRIBUTE TO GALILEO GALILEI, FOUNDER OF MODERN SCIENCE AND TO ENRICO FERMI, THE "ITALIAN NAVIGATOR", FATHER OF THE WEAK FORCES ETTORE MAJORANA CENTENARY ETTORE MAJORANA: GENIUS AND MYSTERY Antonino Zichichi ETTORE MAJORANA: GENIUS AND MYSTERY Antonino Zichichi ABSTRACT The geniality of Ettore Majorana is discussed in the framework of the crucial problems being investigated at the time of his activity. These problems are projected to our present days, where the number of space-time dimensions is no longer four and where the unification of the fundamental forces needs the Majorana particle: neutral, with spin ½ and identical to its antiparticle. The mystery of the way Majorana disappeared is restricted to few testimonies, while his geniality is open to all eminent physicists of the XXth century, who had the privilege of knowing him, directly or indirectly. 3 44444444444444444444444444444444444 ETTORE MAJORANA: GENIUS AND MYSTERY Antonino Zichichi CONTENTS 1 LEONARDO SCIASCIA’S IDEA 5 2 ENRICO FERMI: FEW OTHERS IN THE WORLD COULD MATCH MAJORANA’S DEEP UNDERSTANDING OF THE PHYSICS OF THE TIME 7 3 RECOLLECTIONS BY ROBERT OPPENHEIMER 19 4 THE DISCOVERY OF THE NEUTRON – RECOLLECTIONS BY EMILIO SEGRÉ AND GIANCARLO WICK 21 5 THE MAJORANA ‘NEUTRINOS’ – RECOLLECTIONS BY BRUNO PONTECORVO – THE MAJORANA DISCOVERY ON THE DIRAC γ- MATRICES 23 6 THE FIRST COURSE OF THE SUBNUCLEAR PHYSICS SCHOOL (1963): JOHN BELL ON THE DIRAC AND MAJORANA NEUTRINOS 45 7 THE FIRST STEP TO RELATIVISTICALLY DESCRIBE PARTICLES WITH ARBITRARY SPIN 47 8 THE CENTENNIAL OF THE BIRTH OF A GENIUS – A HOMAGE BY THE INTERNATIONAL SCIENTIFIC COMMUNITY 53 REFERENCES 61 4 44444444444444444444444444444444444 Ettore Majorana’s photograph taken from his university card dated 3rd November 1923. -
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. -
The Germanium Detector Array for the Search of Neutrinoless Double Beta Decay of 76Ge
Colloquium on particle physics, astrophysics and cosmology 22 November 2004 GERDA The GERmanium Detector Array for the search of neutrinoless double beta decay of 76Ge Bernhard Schwingenheuer, Max-Planck-Insitut Kernphysik, Heidelberg Outline o Physics Motivation o Nuclear Matrix Elements oPast 76Ge Experiments o The GERDA Approach o Our Friends: the Competition oSummary GERDA Collaboration INFN LNGS, Assergi, Italy INR, Moscow, Russia A.Di Vacri, M. Junker, M. Laubenstein, C. Tomei, L. Pandola I. Barabanov, L. Bezrukov, A. Gangapshev, V. Gurentsov, V. Kusminov, E. Yanovich JINR Dubna, Russia ITEP Physics, Moscow, Russia S. Belogurov,V. Brudanin, V. Egorov, K. Gusev, S. Katulina, V.P. Bolotsky, E. Demidova, I.V. Kirpichnikov, A.A. A. Klimenko, O. Kochetov, I. Nemchenok, V. Vasenko, V.N. Kornoukhov Sandukovsky, A. Smolnikov, J. Yurkowski, S. Vasiliev, Kurchatov Institute, Moscow, Russia MPIK, Heidelberg, Germany A.M. Bakalyarov, S.T. Belyaev, M.V. Chirchenko, G.Y. C. Bauer, O. Chkvorets, W. Hampel, G. Heusser, W. Grigoriev, L.V. Inzhechik, V.I. Lebedev, A.V. Tikhomirov, Hofmann, J. Kiko, K.T. Knöpfle, P. Peiffer, S. S.V. Zhukov Schönert, J. Schreiner, B. Schwingenheuer, H. Simgen, G. Zuzel MPI Physik, München, Germany I. Abt, M. Altmann, C. Bűttner. A. Caldwell, R. Kotthaus, X. Univ. Köln, Germany Liu, H.-G. Moser, R.H. Richter J. Eberth, D. Weisshaar Univ. di Padova e INFN, Padova, Italy Jagiellonian University, Krakow, Poland A. Bettini, E. Farnea, C. Rossi Alvarez, C.A. Ur M.Wojcik Univ. Tübingen, Germany Univ. di Milano Bicocca e INFN, Milano, Italy M. Bauer, H. Clement, J. Jochum, S. Scholl, K. -
GERDA: Germanium Detector Array Searching for 0Νββ Decay Gedet: Germanium Detector R&D
GERDA: GERmanium Detector Array searching for 0νββ decay GeDet: Germanium Detector R&D Director: Allen Caldwell Projector leaders: Béla Majorovits (GERDA), Iris Abt (GeDet) Postdoc: Josef Janicsko, Xiang Liu, Jens Schubert Ph.D.: Manuela Jelen, Kevin Kröninger(graduated 07/07), Daniel Lenz, Jing Liu Group engineer: Franz Stelzer Diplomand: Markus Kästle Werkstudenten/in: Golam Dastagir, Westa Domanova, Maximilian Empl, Daniel Greenwald, Andreas Kaiser Construction: Karlheinz Ackermann, Stefan Mayer, Sven Voggt Many thanks to colleagues from electronic & mechanic departments! Project Review 17/12/2007 Neutrino masses & mixing parameters 2 ν ν3 2 ν1 Mass 2 e Δm 32 μ ν τ 2 2 Δm 21 ν1 ν3 normal (NH) inverted (IH) 0 2 -3 2 atmospheric accelerator Æ Δm 32 = 2.2•10 eV 2 -5 2 solar reactor Æ Δm 21 = 8.1•10 eV absolute mass NH or IH Dirac or Majorana(ν=ν) page 2 0νββ decay Æ effective Majorana neutrino mass mββ np W- (A,Z) Æ (A, Z+2) + 2e- e- νL ΔL ≠0 e- νR happens, if ν=ν& mν>0 W- n p 2 2 −1 2 GT gV F half life []T1/2 = G( Q,Z)⋅ M − 2 M ⋅ mββ gA Phase space nuclear matrix element effective mass mββ 2 2 2 2 i(α2 −α1) i(−α1−2δ) mββ = ∑mjUej = m1 ⋅ Ue1 +m2 ⋅ Ue2 e +m3 ⋅ Ue3 e j page 3 Measure T1/2 of 0νββ decay npnp W- - e- e ν L ν - e- νR e W- ν n p n p 0νββ 2νββ: (A,Z) Æ (A,Z+2) +2e-+2ν search for energy peak at Q value (Ge76: 2039keV) page 4 0νββ experiments 21 Experiment Underground Isotope T1/2 [10 y] <mee> [eV] (selected) Laboratory Elegant VI Oto (Japan) 48Ca > 95 < 7.2 - 44.7 Heidelberg- Gran Sasso 76Ge >19000 < 0.35 - 1.2 Moscow (Italy) -
Realization of the Low Background Neutrino Detector Double Chooz: from the Development of a High-Purity Liquid & Gas Handling Concept to first Neutrino Data
Realization of the low background neutrino detector Double Chooz: From the development of a high-purity liquid & gas handling concept to first neutrino data Dissertation of Patrick Pfahler TECHNISCHE UNIVERSITAT¨ MUNCHEN¨ Physik Department Lehrstuhl f¨urexperimentelle Astroteilchenphysik / E15 Univ.-Prof. Dr. Lothar Oberauer Realization of the low background neutrino detector Double Chooz: From the development of high-purity liquid- & gas handling concept to first neutrino data Dipl. Phys. (Univ.) Patrick Pfahler Vollst¨andigerAbdruck der von der Fakult¨atf¨urPhysik der Technischen Universit¨atM¨unchen zur Erlangung des akademischen Grades eines Doktors des Naturwissenschaften (Dr. rer. nat) genehmigten Dissertation. Vorsitzender: Univ.-Prof. Dr. Alejandro Ibarra Pr¨uferder Dissertation: 1. Univ.-Prof. Dr. Lothar Oberauer 2. Priv.-Doz. Dr. Andreas Ulrich Die Dissertation wurde am 3.12.2012 bei der Technischen Universit¨atM¨unchen eingereicht und durch die Fakult¨atf¨urPhysik am 17.12.2012 angenommen. 2 Contents Contents i Introduction 1 I The Neutrino Disappearance Experiment Double Chooz 5 1 Neutrino Oscillation and Flavor Mixing 6 1.1 PMNS Matrix . 6 1.2 Flavor Mixing and Neutrino Oscillations . 7 1.2.1 Survival Probability of Reactor Neutrinos . 9 1.2.2 Neutrino Masses and Mass Hierarchy . 12 2 Reactor Neutrinos 14 2.1 Neutrino Production in Nuclear Power Cores . 14 2.2 Energy Spectrum of Reactor neutrinos . 15 2.3 Neutrino Flux Approximation . 16 3 The Double Chooz Experiment 19 3.1 The Double Chooz Collaboration . 19 3.2 Experimental Site: Commercial Nuclear Power Plant in Chooz . 20 3.3 Physics Program and Experimental Concept . 21 3.4 Signal . 23 3.4.1 The Inverse Beta Decay (IBD) . -
In-Situ Gamma-Ray Background Measurements for Next Generation CDEX Experiment in the China Jinping Underground Laboratory a a a a ∗ a a A,B a H
In-situ gamma-ray background measurements for next generation CDEX experiment in the China Jinping Underground Laboratory a a a a < a a a,b a H. Ma , Z. She , W. H. Zeng , Z. Zeng , , M. K. Jing , Q. Yue , J. P. Cheng , J. L. Li and a H. Zhang aKey Laboratory of Particle and Radiation Imaging (Ministry of Education) and Department of Engineering Physics, Tsinghua University, Beijing 100084 bCollege of Nuclear Science and Technology, Beijing Normal University, Beijing 100875 ARTICLEINFO ABSTRACT Keywords: In-situ -ray measurements were performed using a portable high purity germanium spectrometer in In-situ -ray measurements Hall-C at the second phase of the China Jinping Underground Laboratory (CJPL-II) to characterise Environmental radioactivity the environmental radioactivity background below 3 MeV and provide ambient -ray background Underground laboratory parameters for next generation of China Dark Matter Experiment (CDEX). The integral count rate Rare event physics of the spectrum was 46.8 cps in the energy range of 60 to 2700 keV. Detection efficiencies of the CJPL spectrometer corresponding to concrete walls and surrounding air were obtained from numerical calculation and Monte Carlo simulation, respectively. The radioactivity concentrations of the walls 238 232 in the Hall-C were calculated to be 6:8 , 1:5 Bq/kg for U, 5:4 , 0:6 Bq/kg for Th, 81:9 , 14:3 40 Bq/kg for K. Based on the measurement results, the expected background rates from these primordial radionuclides of future CDEX experiment were simulated in unit of counts per keV per ton per year (cpkty) for the energy ranges of 2 to 4 keV and around 2 MeV. -
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 . -
Current and Future Neutrino Experiments
Current and future neutrino experiments Justyna Łagoda XXIV Cracow EPIPHANY Conference on Advances in Heavy Flavour Physics Plan ● short introduction ● non-oscillation experiments – neutrino mass measurements – search for neutrinoless double beta decay ● oscillation experiments – reactor neutrinos – solar neutrinos – atmospheric neutrinos – long baseline experiments – search for sterile neutrinos ● summary 2 Neutrino mixing ● mixing matrix for 3 active flavours −i δ c 0 s e CP 2 additional 1 0 0 13 13 c12 s12 0 phases if νe ν1 ν = 0 c s ⋅ 0 1 0 ⋅ −s c 0 ⋅ ν neutrinos are μ 23 23 12 12 2 Majorana i δ (ντ) CP ν ( 3) particles 0 −s23 c23 −s e 0 c ( 0 0 1) ( )( 13 13 ) ● 3 mixing angles θ12, θ13, θ23, CP violation phase δCP L L P =δ −4 ℜ(U * U U U * )sin2 Δm2 ±2 ℑ(U * U U U * )sin2 Δm2 να →νβ αβ ∑ αi βi α j β j ij ∑ αi βi α j β j ij i>j 4 E i>j 4 E ● 2 2 2 2 2 2 2 independent mass splittings: Δm 21= m 2–m 1, Δm 32 = m 3–m 2, ● 2 “controlled” parameters: baseline L and neutrino energy E ● the presence of matter (electrons) modifies the mixing – energy levels of propagating eigenstates are altered for νe component (different interaction potentials in kinetic part of the hamiltonian) – matter effects are sensitive to ordering of mass eigenstates 3 Known and unknown ● neutrino properties are measured using neutrinos from various sources in various processes and detection techniques −i δ i α /2 c 0 s e CP 1 mixing 1 0 0 13 13 c12 s12 0 e 0 0 i α 2/ 2 parameters: 0 c23 s23 0 1 0 −s12 c12 0 0 e 0 i δCP oscillation 0 −s23 c23 −s e 0 c ( 0 0 1)( 0 -
Arxiv:1509.08702V2 [Physics.Ins-Det] 4 Apr 2016 Be Neutron-Quiet and Suitable for Deployment of the COHERENT Detector Suite
The COHERENT Experiment at the Spallation Neutron Source D. Akimov,1, 2 P. An,3 C. Awe,4, 3 P.S. Barbeau,4, 3 P. Barton,5 B. Becker,6 V. Belov,1, 2 A. Bolozdynya,2 A. Burenkov,1, 2 B. Cabrera-Palmer,7 J.I. Collar,8 R.J. Cooper,5 R.L. Cooper,9 C. Cuesta,10 D. Dean,11 J. Detwiler,10 A.G. Dolgolenko,1 Y. Efremenko,2, 6 S.R. Elliott,12 A. Etenko,13, 2 N. Fields,8 W. Fox,14 A. Galindo-Uribarri,11, 6 M. Green,15 M. Heath,14 S. Hedges,4, 3 D. Hornback,11 E.B. Iverson,11 L. Kaufman,14 S.R. Klein,5 A. Khromov,2 A. Konovalov,1, 2 A. Kovalenko,1, 2 A. Kumpan,2 C. Leadbetter,3 L. Li,4, 3 W. Lu,11 Y. Melikyan,2 D. Markoff,16, 3 K. Miller,4, 3 M. Middlebrook,11 P. Mueller,11 P. Naumov,2 J. Newby,11 D. Parno,10 S. Penttila,11 G. Perumpilly,8 D. Radford,11 H. Ray,17 J. Raybern,4, 3 D. Reyna,7 G.C. Rich∗,3 D. Rimal,17 D. Rudik,1, 2 K. Scholbergy,4, z B. Scholz,8 W.M. Snow,14 V. Sosnovtsev,2 A. Shakirov,2 S. Suchyta,18 B. Suh,4, 3 R. Tayloe,14 R.T. Thornton,14 I. Tolstukhin,2 K. Vetter,18, 5 and C.H. Yu11 1SSC RF Institute for Theoretical and Experimental Physics of National Research Centre \Kurchatov Institute", Moscow, 117218, Russian Federation 2National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Moscow, 115409, Russian Federation 3Triangle Universities Nuclear Laboratory, Durham, North Carolina, 27708, USA 4Department of Physics, Duke University, Durham, NC 27708, USA 5Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA 6Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996, USA 7Sandia -
IUPAP Report 41A
IUPAP Report 41a A Report on Deep Underground Research Facilities Worldwide (updated version of August 8, 2018) Table of Contents INTRODUCTION 3 SNOLAB 4 SURF: Sanford Underground Research Facility 10 ANDES: AGUA NEGRA DEEP EXPERIMENT SITE 16 BOULBY UNDERGROUND LABORATORY 18 LSM: LABORATOIRE SOUTERRAIN DE MODANE 21 LSC: LABORATORIO SUBTERRANEO DE CANFRANC 23 LNGS: LABORATORI NAZIONALI DEL GRAN SASSO 26 CALLIO LAB 29 BNO: BAKSAN NEUTRINO OBSERVATORY 34 INO: INDIA BASED NEUTRINO OBSERVATORY 41 CJPL: CHINA JINPING UNDERGROUND LABORATORY 43 Y2L: YANGYANG UNDERGROUND LABORATORY 45 IBS ASTROPHYSICS RESEARCH FACILITY 48 KAMIOKA OBSERVATORY 50 SUPL: STAWELL UNDERGROUND PHYSICS LABORATORY 53 - 2 - __________________________________________________INTRODUCTION LABORATORY ENTRIES BY GEOGRAPHICAL REGION Deep Underground Laboratories and their associated infrastructures are indicated on the following map. These laboratories offer low background radiation for sensitive detection systems with an external users group for research in nuclear physics, astroparticle physics, and dark matter. The individual entries on the Deep Underground Laboratories are primarily the responses obtained through a questionnaire that was circulated. In a few cases, entries were taken from the public information supplied on the lab’s website. The information was provided on a voluntary basis and not all laboratories included in this list have completed construction, as a result, there are some unavoidable gaps. - 3 - ________________________________________________________SNOLAB (CANADA) SNOLAB 1039 Regional Road 24, Creighton Mine #9, Lively ON Canada P3Y 1N2 Telephone: 705-692-7000 Facsimile: 705-692-7001 Email: [email protected] Website: www.snolab.ca Oversight and governance of the SNOLAB facility and the operational management is through the SNOLAB Institute Board of Directors, whose member institutions are Carleton University, Laurentian University, Queen’s University, University of Alberta and the Université de Montréal. -
Neutrino Oscillations: the Rise of the PMNS Paradigm Arxiv:1710.00715
Neutrino oscillations: the rise of the PMNS paradigm C. Giganti1, S. Lavignac2, M. Zito3 1 LPNHE, CNRS/IN2P3, UPMC, Universit´eParis Diderot, Paris 75252, France 2Institut de Physique Th´eorique,Universit´eParis Saclay, CNRS, CEA, Gif-sur-Yvette, France∗ 3IRFU/SPP, CEA, Universit´eParis-Saclay, F-91191 Gif-sur-Yvette, France November 17, 2017 Abstract Since the discovery of neutrino oscillations, the experimental progress in the last two decades has been very fast, with the precision measurements of the neutrino squared-mass differences and of the mixing angles, including the last unknown mixing angle θ13. Today a very large set of oscillation results obtained with a variety of experimental config- urations and techniques can be interpreted in the framework of three active massive neutrinos, whose mass and flavour eigenstates are related by a 3 3 unitary mixing matrix, the Pontecorvo- × Maki-Nakagawa-Sakata (PMNS) matrix, parameterized by three mixing angles θ12, θ23, θ13 and a CP-violating phase δCP. The additional parameters governing neutrino oscillations are the squared- mass differences ∆m2 = m2 m2, where m is the mass of the ith neutrino mass eigenstate. This ji j − i i review covers the rise of the PMNS three-neutrino mixing paradigm and the current status of the experimental determination of its parameters. The next years will continue to see a rich program of experimental endeavour coming to fruition and addressing the three missing pieces of the puzzle, namely the determination of the octant and precise value of the mixing angle θ23, the unveiling of the neutrino mass ordering (whether m1 < m2 < m3 or m3 < m1 < m2) and the measurement of the CP-violating phase δCP. -
Majorana Returns Frank Wilczek in His Short Career, Ettore Majorana Made Several Profound Contributions
perspective Majorana returns Frank Wilczek In his short career, Ettore Majorana made several profound contributions. One of them, his concept of ‘Majorana fermions’ — particles that are their own antiparticle — is finding ever wider relevance in modern physics. nrico Fermi had to cajole his friend Indeed, when, in 1928, Paul Dirac number of electrons minus the number of Ettore Majorana into publishing discovered1 the theoretical framework antielectrons, plus the number of electron Ehis big idea: a modification of the for describing spin-½ particles, it seemed neutrinos minus the number of antielectron Dirac equation that would have profound that complex numbers were unavoidable neutrinos is a constant (call it Le). These ramifications for particle physics. Shortly (Box 2). Dirac’s original equation contained laws lead to many successful selection afterwards, in 1938, Majorana mysteriously both real and imaginary numbers, and rules. For example, the particles (muon disappeared, and for 70 years his modified therefore it can only pertain to complex neutrinos, νμ) emitted in positive pion (π) + + equation remained a rather obscure fields. For Dirac, who was concerned decay, π → μ + νμ, will induce neutron- − footnote in theoretical physics (Box 1). with describing electrons, this feature to-proton conversion νμ + n → μ + p, Now suddenly, it seems, Majorana’s posed no problem, and even came to but not proton-to-neutron conversion + concept is ubiquitous, and his equation seem an advantage because it ‘explained’ νμ + p → μ + n; the particles (muon is central to recent work not only in why positrons, the antiparticles of antineutrinos, ν¯ μ) emitted in the negative − − neutrino physics, supersymmetry and dark electrons, exist.