Generation Mixing and CP-Violation - Standard and Beyond*
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The Structure of Quarks and Leptons
The Structure of Quarks and Leptons They have been , considered the elementary particles ofmatter, but instead they may consist of still smaller entities confjned within a volume less than a thousandth the size of a proton by Haim Harari n the past 100 years the search for the the quark model that brought relief. In imagination: they suggest a way of I ultimate constituents of matter has the initial formulation of the model all building a complex world out of a few penetrated four layers of structure. hadrons could be explained as combina simple parts. All matter has been shown to consist of tions of just three kinds of quarks. atoms. The atom itself has been found Now it is the quarks and leptons Any theory of the elementary particles to have a dense nucleus surrounded by a themselves whose proliferation is begin fl. of matter must also take into ac cloud of electrons. The nucleus in turn ning to stir interest in the possibility of a count the forces that act between them has been broken down into its compo simpler-scheme. Whereas the original and the laws of nature that govern the nent protons and neutrons. More recent model had three quarks, there are now forces. Little would be gained in simpli ly it has become apparent that the pro thought to be at least 18, as well as six fying the spectrum of particles if the ton and the neutron are also composite leptons and a dozen other particles that number of forces and laws were thereby particles; they are made up of the small act as carriers of forces. -
LIMITS on DIFFERENT MAJORON DECAY MODES of 100Mo, 116Cd, 82Se, and 96Zr for NEUTRINOLESS DOUBLE BETA DECAYS in the NEMO-2 EXPERIMENT V
XJ0200048 B 3HAJL 2001. N»5[108] Particles and Nuclei, Letters. 2001. No.5[108] 539.165 LIMITS ON DIFFERENT MAJORON DECAY MODES OF 100Mo, 116Cd, 82Se, AND 96Zr FOR NEUTRINOLESS DOUBLE BETA DECAYS IN THE NEMO-2 EXPERIMENT V. Vasilyev et al. (NEMO collaboration1) The NEMO-2 tracking detector located in the Frejus underground laboratory was designed as a prototype for the NEMO-3 detector and to study different modes of double beta decay. Measurements with 100Mo, n6Cd, 82Se, and 96Zr were carried out. Presented here are the experimental half-life limits on double beta decays for new Majoron emission modes and limits on effective neutrino-Majoron coupling constants. NEMO-2, pacnario>KeHHbiH B nofl3eMHOH jiaSopaTopHH ©peaxyc H CKOHcrpynpoBaH- HHH KaK npoTOTHn aeTeKTopa NEMO-3, npeflHa3HaieH ana H3vqeHHa pa3HHHHbix MOB flBoflHoro 6era- pacnaaa. EbuiH npoBeaeHbi H3MepeHHs H3oronoB 100Mo, U6Cd, 82Se H 96Zr. B pa6oTe npeflcraBJieHbi HOBbie 3KcnepHMenTanbHbie npeaenu Ha pa3nnHHbie MOflbi flBOHHoro 6eTa-pacnana c HcnycKaHweM Mafl- OpOHa H 3CpcbeKTHBHb]X K0HCT8HT CBH3H HeHTpHHO-MaHOpOH. INTRODUCTION Spontaneous violation of global (B—L) symmetry in gauge theories leads to the existence of a massless Goldstone boson, the Majoron. At the beginning of the 1980's there were considered to be singlet [1], doublet [2] and triplet [3] Majoron models. All these models resulted in the neutrinoless double beta (2/3) decay with the emission of a Majoron (x°): (A,Z)-+(A,Z + 2) + 2e-+x°- (D However, the interaction of the triplet (or doublet) Majorons with the Z° boson would give a contribution to the width of the Z° decay, which corresponds to two (or 1/2) additional massless neutrino types (see, for example, [4-6]). -
Israel Prize
Year Winner Discipline 1953 Gedaliah Alon Jewish studies 1953 Haim Hazaz literature 1953 Ya'akov Cohen literature 1953 Dina Feitelson-Schur education 1953 Mark Dvorzhetski social science 1953 Lipman Heilprin medical science 1953 Zeev Ben-Zvi sculpture 1953 Shimshon Amitsur exact sciences 1953 Jacob Levitzki exact sciences 1954 Moshe Zvi Segal Jewish studies 1954 Schmuel Hugo Bergmann humanities 1954 David Shimoni literature 1954 Shmuel Yosef Agnon literature 1954 Arthur Biram education 1954 Gad Tedeschi jurisprudence 1954 Franz Ollendorff exact sciences 1954 Michael Zohary life sciences 1954 Shimon Fritz Bodenheimer agriculture 1955 Ödön Pártos music 1955 Ephraim Urbach Jewish studies 1955 Isaac Heinemann Jewish studies 1955 Zalman Shneur literature 1955 Yitzhak Lamdan literature 1955 Michael Fekete exact sciences 1955 Israel Reichart life sciences 1955 Yaakov Ben-Tor life sciences 1955 Akiva Vroman life sciences 1955 Benjamin Shapira medical science 1955 Sara Hestrin-Lerner medical science 1955 Netanel Hochberg agriculture 1956 Zahara Schatz painting and sculpture 1956 Naftali Herz Tur-Sinai Jewish studies 1956 Yigael Yadin Jewish studies 1956 Yehezkel Abramsky Rabbinical literature 1956 Gershon Shufman literature 1956 Miriam Yalan-Shteklis children's literature 1956 Nechama Leibowitz education 1956 Yaakov Talmon social sciences 1956 Avraham HaLevi Frankel exact sciences 1956 Manfred Aschner life sciences 1956 Haim Ernst Wertheimer medicine 1957 Hanna Rovina theatre 1957 Haim Shirman Jewish studies 1957 Yohanan Levi humanities 1957 Yaakov -
Neutrinoless Double-Β Decay with Nonstandard Majoron Emission
PHYSICAL REVIEW LETTERS 122, 181801 (2019) Neutrinoless Double-β Decay with Nonstandard Majoron Emission † ‡ ∥ Ricardo Cepedello,1,2,* Frank F. Deppisch,2,3, Lorena González,4,2, Chandan Hati,5,§ and Martin Hirsch1, 1AHEP Group, Instituto de Física Corpuscular—CSIC/Universitat de Val`encia Edificio de Institutos de Paterna, Apartado 22085, E–46071 Val`encia, Spain 2Department of Physics and Astronomy, University College London, London WC1E 6BT, United Kingdom 3Institut für Hochenergiephysik, Österreichische Akademie der Wissenschaften, Nikolsdorfer Gasse 18, 1050 Wien, Austria 4Department of Physics, Universidad T´ecnica Federico Santa María, Avenida España 1680, Valparaíso, Chile 5Laboratoire de Physique de Clermont, CNRS/IN2P3 UMR 6533, Campus des C´ezeaux, 4 Avenue Blaise Pascal, F-63178 Aubi`ere Cedex, France (Received 13 November 2018; revised manuscript received 1 February 2019; published 7 May 2019) We present a novel mode of neutrinoless double-β decay with emission of a light Majoron-like scalar particle ϕ. We assume it couples via an effective seven-dimensional operator with a (V þ A) lepton current and (V Æ A) quark currents leading to a long-range contribution that is unsuppressed by the light neutrino mass. We calculate the total double-β decay rate and determine the fully differential shape for this mode. β Λ ≈ 1 We find that future double- decay searches are sensitive to scales of the order NP TeV for the effective operator and a light scalar mϕ < 0.2 MeV, based on ordinary double-β decay Majoron searches. The angular and energy distributions can deviate considerably from that of two-neutrino double-β decay, which is the main background. -
Some Consequences of the Majoron Being the Dark Radiation ∗ We-Fu Chang A,B,Johnn.Ngc, Jackson M.S
Physics Letters B 730 (2014) 347–352 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Some consequences of the Majoron being the dark radiation ∗ We-Fu Chang a,b,JohnN.Ngc, Jackson M.S. Wu a,b, a Department of Physics, National Tsing Hua University, No. 101, Section 2, Kuang-Fu Road, Hsinchu, 30013, Taiwan, ROC b Physics Division, National Center for Theoretical Sciences, No. 101, Section 2, Kuang-Fu Road, Hsinchu, 30013, Taiwan, ROC c TRIUMF, 4004 Wesbrook Mall, Vancouver, BC, V6T 2A3, Canada article info abstract Article history: We discuss some phenomenological consequences in a scenario where a singlet Majoron plays the role Received 1 November 2013 of dark radiation. We study the interrelations between neutrino mass generation and the scalar potential Received in revised form 12 December 2013 arising from this identification. We find the extra scalar has to be light with a mass at or below the Accepted 29 January 2014 GeV level. The mixing of this scalar with the Standard Model Higgs impacts low energy phenomena such Available online 11 February 2014 as the muonic hydrogen Lamb shift and muon anomalous magnetic moment. Demanding that the light Editor: S. Dodelson scalar solves the puzzle in the muon magnetic moment requires the scalar to be lighter still with mass at or below the 10 MeV level. The cross-sections for the production of heavy neutrinos at LHC14 are also given. © 2014 Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/3.0/). -
Braided Fermions from Hurwitz Algebras
Braided fermions from Hurwitz algebras Niels G Gresnigt Xi'an Jiaotong-Liverpool University, Department of Mathematical Sciences. 111 Ren'ai Road, Dushu Lake Science and Education Innovation District, Suzhou Industrial Park, Suzhou, 215123, P.R. China E-mail: [email protected] Abstract. Some curious structural similarities between a recent braid- and Hurwitz algebraic description of the unbroken internal symmetries for a single generations of Standard Model fermions were recently identified. The non-trivial braid groups that can be represented using c the four normed division algebras are B2 and B3, exactly those required to represent a single generation of fermions in terms of simple three strand ribbon braids. These braided fermion states can be identified with the basis states of the minimal left ideals of the Clifford algebra C`(6), generated from the nested left actions of the complex octonions C ⊗ O on itself. That is, the ribbon spectrum can be related to octonion algebras. Some speculative ideas relating to ongoing research that attempts to construct a unified theory based on braid groups and Hurwitz algebras are discussed. 1. Introduction Leptons and quarks are identified with representations of the gauge group U(1)Y × SU(2)L × SU(3)C in the Standard Model (SM) of particle physics. Despite its success in accurately describing and predicting experimental observations, this gauge group lacks a theoretical basis. Why has Nature chosen these gauge groups from an infinite set of Lie groups, and why do only some representations correspond to physical states? A second shortcoming of the SM is the lack of gravity, or equivalently, its unification with General Relativity (GR). -
Majorons and Supernova Cooling
Novell).ber 29, 1989 CMU-HEP89-23 MPI-PAE/PTh 75/89 ' Majorons and Supernova Cooling 1 2 Kiwoon Choi ) and A. Santan1aria* ) 1 ) Department of Physics, Carnegie Mellon University Pittsburgh, PA 15213, USA 2 ) Max-Planck-Institut fiir Physik und Astrophysik Fahringer Ring 6, D-8000 Miinchen 40, Germany Abstract We consider the role of majoron emission in supernova cooling and its implications for the neutrino mass and lifetime in generic singlet majoron models. It is found that for v, with mass m, if the lifetime for the decay v, ...... majoron + v .... is shorter than 10-7(m/MeV) sec, then majorons are so strongly trapped by the inverse process that the resulting majoron luminosity is small enough to not destabilize the observed v.-pulse from SN1987 A. For v, with a longer lifetime, the majoron luminosity can be large enough to destroy or significantly shorten the duration of the neutrino pulse. We then find the range of paran1eters, e.g. the v,-mass m and the B- L breaking scale v, that is excluded by giving such a large majoron luminosity. Our results imply that, for v between 1 GeV and 1 TeV, a wide range of m allowed by terrestrial experiments can be excluded in view of the observed v.-pulse from SN1987 A. *Permanent address: Departament de Fisica TeOrica, Universitat de Valencia and IFIC, Universitat de Valencia-CSIC, Spain. 1. Introduction The supernova SN1987 All] in the Large Magelanic Cloud has provided a lot of information on the properties of neutrinos, e.g. masses, number of generationsl2l, mag 3 4 8 netic momentsl l, and exotic interactionsl - l. -
RESULTS Haim Harari Weizmann Institute of Science, Rehovot, Israel and Stanford Linear Accele
THEORETICAL INTERPRETATION OF e+e- RESULTS Haim Harari Weizmann Institute of Science, Rehovot, Israel and Stanford Linear Accelerator Center, Stanford University Stanford, California, U.S.A. Summary First Generation Fermions: Are quarks and leptons Recent experimental results and theoretical ideas pointlike? Do quarks come in three colors? Do they related to e+e- scattering are reviewed. have the "usual" charges of i and - j-? Second Generation Fermions: Is the right-handed muon 1. INTRODUCTION: A Long List of Answerable Questions in an SU(2) x U(l) singlet? Is the cs current a V-A The study of electron-positron collisions has current? What is the cc potential? Where are the gradually become the most productive experimental pseudoscalar charmonium states? Do semileptonic D-decays method of uncovering new particles and new phenomena. proceed mainly to strange particles, as predicted by Beginning with the "November revolution" of 1974 and GIM? What are the features of nonleptonic D-decays? continuing at an incredibly rapid pace since that What are the properties of F+, A+ , L etc? time, the 1JJ family, the T-lepton, the D+ and DO, c c Third Generation Fermions: Does the top quark exist, various D*'s and possibly F+ were discovered in e+e and if so, what is its mass? Do B-mesons and T-mesons collisions, while the T-states, the charmed baryons as exist? Are the charged currents involving t and b, well as quark jets and now gluon jets have been studied. left-handed? What are the values of the generalized Our present theoretical picture of the fundamental Cabibbo angles 8 ,8 and the Kobayashi-Maskawa phase particles and their interactions is very compact. -
Arxiv:Hep-Ph/9309214V1 2 Sep 1993 Etitosfo H Oeeprmn.I Rvdsa Poss at a Line As X-Ray Provides an It of Experiment
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Repositori d'Objectes Digitals per a l'Ensenyament la Recerca i la Cultura FTUV/93-35 December 21, 2013 Submitted to Phys. Lett. B The KeV Majoron as a Dark Matter Particle V. Berezinsky 1 INFN, Laboratori Nazionali del Gran Sasso I-67010, Assergi (AQ), Italy and Institute for Nuclear Research, Moscow, Russia and J. W. F. Valle 2 Instituto de Fisica Corpuscular - IFIC/CSIC Dept. de F´isica Te`orica, Universitat de Val`encia 46100 Burjassot, Val`encia, SPAIN ABSTRACT We consider a very weakly interacting KeV majoron as a dark matter particle (DMP), which provides both the critical density ρ = 1.88 10 29h2 g/cm3 and the galactic scale cr × − 3 2 12 2 Mgal mP l/mJ 10 M (mJ /1KeV )− for galaxy formation. The majoron couples ∼ ∼ ⊙ to the leptons only through some new ”directly interacting particles”, called DIPS, and this provides the required smallness of the coupling constants. If the masses of these DIPS are greater than the scale Vs characterizing the spontaneous violation of the global lepton symmetry they are absent at the corresponding phase transition (T V ) and the ∼ s arXiv:hep-ph/9309214v1 2 Sep 1993 majorons are produced during the phase transition, never being in thermal equilibrium during the history of the universe. In the alternative case mDIP < Vs the majorons can be for a short period in thermal equilibrium. This scenario is not forbidden by nucleosynthesis and gives a reasonable growth factor for the density fluctuations compatible with the recent restrictions from the COBE experiment. -
Neutrino Lines from Majoron Dark Matter
Neutrino Lines from Majoron Dark Matter PoS(NuFact2017)138 Julian Heeck∗ Service de Physique Théorique, Université Libre de Bruxelles, CP225, 1050 Brussels, Belgium E-mail: [email protected] Majorons are the Goldstone bosons associated to lepton number and thus closely connected to Majorana neutrino masses. At tree level, its only fermion couplings are to neutrinos. Couplings to charged fermions arise at one-loop level, including lepton-flavor-violating ones that lead to decays ` ! `0J, whereas a coupling to photons is generated at two loops. The typically small couplings make massive majorons a prime candidate for long-lived dark matter. Its signature decay into two mono-energetic neutrinos is potentially detectable for majoron masses above MeV and most importantly depends on different parameters than the visible decay channels. The 19th International Workshop on Neutrinos from Accelerators-NUFACT2017 25-30 September, 2017 Uppsala University, Uppsala, Sweden ∗Speaker. c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). https://pos.sissa.it/ Neutrino Lines from Majoron Dark Matter Julian Heeck 1. Majoron couplings We start our discussion with a basic introduction to the majoron model, based on Refs. [1, 2], before delving into the phenomenology of majorons as dark matter (Sec. 2) and the connection to lepton flavor violation (Sec. 3) The difference between baryon number B and lepton number L is an anomaly-free global symmetry of the Standard Model (SM); spontaneously breaking this U(1)B−L symmetry results in a Goldstone boson called majoron [3, 4]. -
The Majoron PALS 27-09-19 3 the Hubble Tension
Could the H0 Tension be Pointing Toward the Neutrino Mass Mechanism? Miguel Escudero Abenza [email protected] based on ArXiv:1909.04044 with Sam Witte PALS Paris 27/09/19 H0 H0 ⌫ ⌫ e ! µ m =0 ⌫ 6 H0 ⌫ ⌫e ⌫µ ⌫¯ ! m =0 φ ⌫ 6 Outline 1) The Hubble Tension 2) The Scenario 3) Cosmology with a light Majoron 4) Conclusions Miguel Escudero (KCL) H0 and the Majoron PALS 27-09-19 3 The Hubble Tension Taken from Wendy Freedman, see 1706.02739 Miguel Escudero (KCL) H0 and the Majoron PALS 27-09-19 4 The Hubble Tension Taken from Wendy Freedman, see 1706.02739 Riess et al 1903.07603 1 1 H = 74.03 1.42 km s− Mpc− 0 ± 4.4 σ tension within ΛCDM! 1 1 H = 67.36 0.54 km s− Mpc− 0 ± Planck 2018 1807.06209 Miguel Escudero (KCL) H0 and the Majoron PALS 27-09-19 4 The Hubble Tension Taken from Wendy Freedman, see 1706.02739 Riess et al 1903.07603 1 1 H = 74.03 1.42 km s− Mpc− 0 ± 4.4 σ tension within ΛCDM! 1 1 H = 67.36 0.54 km s− Mpc− 0 ± Planck 2018 1807.06209 Tension very unlikely generated by CMB systematics see e.g. Spergel et al 1312.3313, Addison et al 1511.00055, Verde et al 1601.01701, Planck 1608.02487 Miguel Escudero (KCL) H0 and the Majoron PALS 27-09-19 4 The Hubble Tension Taken from Wendy Freedman, see 1706.02739 Riess et al 1903.07603 1 1 H = 74.03 1.42 km s− Mpc− 0 ± 4.4 σ tension within ΛCDM! 1 1 H = 67.36 0.54 km s− Mpc− 0 ± Planck 2018 1807.06209 Tension very unlikely generated by CMB systematics see e.g. -
How Gravity Shapes the Low-Energy Frontier of Particle Physics: Neutrino Masses and the Domestic Axion
HOW GRAVITY SHAPES THE LOW-ENERGY FRONTIER OF PARTICLE PHYSICS Neutrino Masses and the Domestic Axion Lena Funcke M ¨unchen2018 HOW GRAVITY SHAPES THE LOW-ENERGY FRONTIER OF PARTICLE PHYSICS Neutrino Masses and the Domestic Axion Dissertation an der Fakultät für Physik der Ludwig–Maximilians–Universität München vorgelegt von Lena Funcke aus Münster München, den 30. Mai 2018 Dissertation an der Fakultät für Physik der Ludwig-Maximilians-Universität München vorgelegt von Lena Funcke am 30. Mai 2018. Erstgutachter: Prof. Dr. Georgi Dvali Zweitgutachter: PD Dr. Georg Raffelt Tag der mündlichen Prüfung: 9. Juli 2018 Max-Planck-Institut für Physik, München, den 30. Mai 2018. Zusammenfassung Das Standardmodell der Teilchenphysik und seine kosmologischen Impli- kationen lassen einige fundamentale Fragen unbeantwortet, insbesondere die Abwesenheit von CP -Verletzung in der starken Wechselwirkung sowie die Ursprünge von Neutrinomassen, Dunkler Materie und Dunkler Energie. Inner- halb der Modellentwicklung jenseits des Standardmodells konzentrieren sich die populärsten Forschungsrichtungen üblicherweise auf neue Strukturen bei hohen Energien bzw. kleinen Abständen. Als eine alternative Richtung präsen- tieren wir in dieser Dissertation eine neue Klasse von niederenergetischen Lösungen der Neutrinomassen- und starken CP -Probleme. Diese Klasse mani- festiert sich auf einer neuen infraroten Gravitationsskala, welche numerisch übereinstimmt mit der Skala der Dunklen Energie. Wir zeigen, wie sich ein Neutrinokondensat, kleine Neutrinomassen und ein Axion aus einer topolo- gischen Formulierung der chiralen Gravitationsanomalie ergeben können. Zuerst rekapitulieren wir, wie ein gravitativer θ-Term zur Entstehung eines 0 neuen gebundenen Neutrinozustands ην führt, analog zum η -Meson in der QCD. Auf dieser Basis leiten wir her, dass sich ein niederenergetisches Neutrino- Vakuumskondensat bildet, welches kleine Neutrinomassen generiert.