Exotic Charges, Multicomponent Dark Matter and Light Sterile Neutrinos
|
|
- Erik Pearson
- 6 years ago
- Views:
Transcription
1 Exotic Charges, Multicomponent and Light Sterile Neutrinos Julian Heeck Max-Planck-Institut für Kernphysik, Heidelberg based on J.H., He Zhang, arxiv:1210.xxxx.
2 Sterile Neutrinos Hints for ev sterile neutrino Neutrino Experiments: LSND (ν µ ν e ): 3.8σ excess at low energies: m 2 LSND 1 ev2 (3 + 1 scheme). MiniBooNE pre 2012: ν µ ν e compatible with LSND, ν µ ν e not CP-violation (3 + 2 scheme). Short baseline reactor experiments (reevaluation of fluxes). Gallium anomaly. sterile neutrino(s) with m s 1 ev and large mixing U as = O(0.1). MiniBooNE 2012: ν µ ν e compatible with ν µ ν e. ICARUS 2012: New bounds on active-sterile mixing: U as < Agreement with LSND worsens... Very fast and exciting field! No need for anymore? Wait for global fits? Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 1 / 18
3 Sterile Neutrinos Hints for ev sterile neutrino II Cosmology: Light d.o.f. in ΛCDM: BBN, CMB and LSS: N s al., JCAP (2011)] BUT, for 3 + 1: m s 0.5 ev at 95%. [Hamann et al., PRL (2010)] Assumes thermalized ν s (makes sense for large mixing). Extend ΛCDM? No thermalization? Wait for Planck? Let s embrace the hints! 0.6. [Hamann et Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 2 / 18
4 Sterile Neutrinos How to make ν s light? Isn t new physics always at TeV? Just put it in: ev-seesaw ( ) 0 md M = m T D M R with m D 0.1 ev, M R 1 ev. [de Gouvêa, PRD (2005)] Active-sterile mixing automatically large: U as m D /M R m ν /m s 0.1. Minimal scheme: two ν R at ev scale, works fine. [Donini, Schwetz et al., JHEP (2012)] The heavy ev-scale suppresses the light 0.1 ev? Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 3 / 18
5 Sterile Neutrinos How to make ν s light? II Put ν s on the other side of the seesaw: ν α ν s ν R Suppressed BY seesaw: additional singlet S, mass matrix for (ν α, ν c R,j, S c ) 0 m D 0 M MES = md T M R m S. 0 ms T 0 Minimal Extended Seesaw (MES) [Barry, Rodejohann, Zhang, JHEP (2011)][Zhang, PLB (2012)] Works also for 3 + 2, 3 + 3,..., just add more singlets. Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 4 / 18
6 Sterile Neutrinos Minimal extended seesaw 0 m D 0 M MES = md T M R m S 0 ms T 0 Assume M R m D, m S, usual seesaw: ( md M 1 M 4 4 ν For m S m D, one more seesaw: and M 3 3 ν m D M 1 R m S ms T M 1 R mt D ms T M 1 R m S R mt D m D M 1 R ). mt D + m D M 1 m S (ms T M 1 m S) 1 ms T M 1 R m 4 m s m T S M 1 R m S. R R mt D Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 5 / 18
7 Mixing Sterile Neutrinos Diagonalize M 4 4 ν with ( (1 1 V 2 RR )U PMNS R R U PMNS R R ), active sterile mixing vector R = m D M 1 R m S (ms T M 1 R m S) 1 O(m D /m S ). m D 100 GeV, m S 500 GeV and M R GeV give m ν 0.05 ev, m s 1.3 ev, R 0.2 Great, but how to get MES structure? Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 6 / 18
8 How to get MES Sterile Neutrinos Need and forbid couplings L H ν R, m S S c ν R, M R ν c R ν R L H S, S c S. Flavor symmetry A 4 Z 4. [Zhang, PLB (2012)] Global U(1) : Y (S) = 1, new scalar φ with Y (φ) = +1: wφs c ν R w φ S }{{} ν R m S Goldstone boson problematic? Contributes 4/7 neutrino species to BBN, so together with ν s : N eff = 11/ Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 7 / 18
9 Local U(1) Sterile Neutrinos More interesting: gauge the U(1) : need more chiral fermions S j to cancel anomalies n Y (S j ) = 0 j and n (Y (S j )) 3 = 0. j make all new particles massive via φ. Try n = 2: Y (S 1 )! = Y (S 2 ), allows M S c 1 S MES only if M 1 ev. bare mass terms are bad... same for n = 3, 4. For n 5, exotic charges open up: Y (S i ) Y (S j ), i, j = 1,..., n. [Babu, Seidl, PLB (2004)] E.g. (10, 4, 9, 2, 7) or ( 5, 5, 1, 6, 2, 3). Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 8 / 18
10 Magic numbers Sterile Neutrinos Try n = 7, i.e. ten right-handed neutrinos : ν R,1 ν R,2 ν R,3 S 1 S 2 S 3 S 4 S 5 S 6 S 7 φ Y Mass matrix has nice block structure: ( ) (MMES ) M = (M S ) 6 6 with 0 y 1 φ y 1 φ M S = y 2 φ y 2 φ y 3 φ y 3 φ 0. S 1 gives MES, S 2,3,4,5,6,7 decouple and form 3 Dirac fermions Ψ 1,2,3! Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 9 / 18
11 More numbers Sterile Neutrinos Happy accident : φ breaks U(1) to Z 11. all three Ψ j stable! Active-sterile mixing V 4j O(m D /m S )! = O(0.1). For O(1) Yukawas U(1) breaking at φ 10 H TeV. masses for Z, Re(φ), Ψ 1,2,3 around 100 GeV TeV. No U(1) Landau pole below M Pl : g Multicomponent WIMP dark matter. Breakdown of neutral fermions: ν e, ν µ, ν τ, S 1, S 2, S 3, S }{{}}{{} 4, S 5, S }{{} 6, S 7, }{{} ν R,1, ν R,2, ν R,3 }{{} (3+1) MES Ψ 1 } Ψ 2 Ψ 3 {{} seesaw/leptogenesis DM Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 10 / 18
12 Sterile Neutrinos Dark matter interactions Lagrangian: ( [iψ j γ µ µ Ψ j M j 1 + Re(φ) ) Re(φ) j Ψ j Ψ j + g 2 Z µψ j γ µ ( gj V + g A j γ 5 ) Ψj ] with g V 1 = 1, g V 2 = 13, g V 3 = 7, g A 1 = 11, g A 2 = 11, g A 3 = 11. Connection to the Standard Model just like all other U(1) DM models: Scalar mixing (Higgs portal): L δ H 2 φ 2 Ψ j couple to Higgs. [Lopez-Honorez et al., PLB (2012)] Vector mixing (kinetic-mixing portal): L sin ξ F µν Y F µν Ψ j couple to Z boson. [Mambrini, JCAP (2011)] New: Fermion mixing (neutrino portal): L 11g 2 Z µ 4 V4iV 4j (ν i γ µ γ 5 ν j + ν i γ µ ν j ). i,j=1 Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 11 / 18
13 Neutrino portal Sterile Neutrinos M R GeV ν R,j φ Z, φ DM : Ψ i Ψ j TeV Z Z H φ H 100 GeV SM Z ev W, Z, H ν α V 4j ν s Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 12 / 18
14 Relic density Sterile Neutrinos Large active-sterile mixing sterile neutrinos are thermalized (probably... ) Z interactions νν ΨΨ thermalize Ψ j. At T < M j, Ψ j annihilates away into lighter Ψ and neutrinos. Freeze-out of lightest Ψ j near Z resonance gives Ωh M = M = M = 800 GeV M = 1 TeV M = M = M = 800 GeV M = 500 GeV 10 0 h h M Z' [GeV] M Z' [GeV] Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 13 / 18
15 Sterile Neutrinos Neutrino portal DM phenomenology 10 1 M = 600 GeV M = 800 GeV M = 1 TeV 10 0 M = 1 TeV 10 1 M = 600 GeV M = 800 GeV 10 0 M = 1 TeV M = 500 GeV h h M Z' [GeV] M Z' [GeV] For M i M j : multicomponent aspect interesting, e.g. coannihilation Ψ j Ψ j Z, φ Ψ i Ψ i. Direct detection is loop-suppressed: m 2 41 /(100 GeV) Indirect detection: BR(ΨΨ νν) 100% gives monochromatic neutrinos from Galactic halo. Too small for IceCube... Including Higgs portal and kinetic-mixing portal gives the usual measurable effects. Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 14 / 18
16 Neutrino portal Sterile Neutrinos M R GeV ν R,j φ Z, φ DM : Ψ i Ψ j TeV Z Z H φ H 100 GeV SM Z ev W, Z, H ν α V 4j ν s Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 15 / 18
17 Sterile Neutrinos Other charges: ν R,1 ν R,2 ν R,3 ν R,4 S 1 S 2 S 3 S 4 S 5 S 6 φ Y Same number of right-handed neutrinos, different decomposition. Only two Dirac DM particles, independently stable by U(1) Z 5. Same qualitative phenomenology. ν e, ν µ, ν τ, S 1, S 2, S 3, S 4, S }{{}}{{} 5, S 6, ν }{{} R,1, ν R,2, ν R,3, ν R,4 }{{} (3+2) MES Ψ 1 } Ψ 2 {{} seesaw/leptogenesis DM Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 16 / 18
18 Sterile Neutrinos Other charges: Unstable dark matter ν R,1 ν R,2 ν R,3 S 1 S 2 S 3 S 4 S 5 S 6 S 7 φ Y ν e, ν µ, ν τ, S 1, S 2, S 3, S }{{}}{{} 4, S 5, S }{{} 6, S 7, }{{} ν R,1, ν R,2, ν R,3 }{{} (3+1) MES Ψ 1 } Ψ 2 Ψ 3 {{} seesaw/leptogenesis DM Breakdown U(1) Z N not a generic feature. Here: only accidental global U(1) 3 symmetry protecting Ψ j. Broken to U(1) by higher-dimensional operators φ 2 S 3 S c 4 /Λ, φ 2 S c 3S 6 /Λ, φ 2 S 2 S c 7 /Λ. Completely broken at even higher order, e.g. φ 6 S 5 ν c R /Λ5. Suppressed DM decay. Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 17 / 18
19 Summary Sterile Neutrinos Additional right-handed neutrinos with exotic charges under a broken U(1) can generate structure in neutral fermions. Here: generate seesaw-suppressed sterile neutrino. Magic numbers: anomaly-cancelling fermions form multicomponent WIMPs. Gauge interactions open new SM-DM portal through thermalized sterile neutrinos. Huge unexplored playground! Other charges: 3 + 2, 3 + 3, Majorana DM, unstable DM,... Julian Heeck - MPIK Exotic Charges, Multicomponent DM and Light Sterile Neutrinos 18 / 18
Neutrinos and Abelian Gauge Symmetries
Neutrinos and Abelian Gauge Symmetries Julian Heeck 24.10.2014 ULB Standard Model of Particle Physics Beautiful and simple: Julian Heeck Neutrinos and Abelian Gauge Symmetries 1/ 43 Standard Model of Particle
More informationGauged Flavor Symmetries
Gauged Flavor Symmetries NOW 2012 Julian Heeck Max-Planck-Institut für Kernphysik, Heidelberg 15.9.2012 based on J.H., Werner Rodejohann, PRD 84 (2011), PRD 85 (2012); Takeshi Araki, J.H., Jisuke Kubo,
More informationFlavor Models with Sterile Neutrinos. NuFact 11 Geneva, Aug, He Zhang
Flavor Models with Sterile Neutrinos NuFact 11 Geneva, Aug, 2011 Contents: Sterile neutrinos in ν-osc. and 0νββ decays Mechanisms for light sterile neutrino masses Flavor symmetry with sterile neutrinos
More informationNeutrino Masses and Dark Matter in Gauge Theories for Baryon and Lepton Numbers
Neutrino Masses and Dark Matter in Gauge Theories for Baryon and Lepton Numbers DPG Frühjahrstagung 014 in Mainz Based on Phys. Rev. Lett. 110, 31801 (013), Phys. Rev. D 88, 051701(R) (013), arxiv:1309.3970
More informationNovember 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model
Scalar from November 24, 2014 1 2 3 4 5 What is the? Gauge theory that explains strong weak, and electromagnetic forces SU(3) C SU(2) W U(1) Y Each generation (3) has 2 quark flavors (each comes in one
More informationTeV Scale Seesaw with Loop Induced
TeV Scale Seesaw with Loop Induced Dirac Mass Term and Dark kmtt Matter from U(1) B L Gauge Symmetry Breaking Takehiro Nabeshima University of Toyama S. Kanemura, T.N., H. Sugiyama, Phys. Lett. B703:66-70
More informationStatus of Light Sterile Neutrinos Carlo Giunti
C. Giunti Status of Light Sterile Neutrinos EPS-HEP 05 3 July 05 /5 Status of Light Sterile Neutrinos Carlo Giunti INFN, Sezione di Torino and Dipartimento di Fisica, Università di Torino giunti@to.infn.it
More informationCosmological constraints on the Sessaw Scale
Cosmological constraints on the Sessaw Scale Jacobo López-Pavón 50th Rencontres de Moriond EW La Thuile, Valle d'aosta (Italy) 14-21 March, 2015 Motivation Which is the simplest extension of the SM that
More informationConstraining minimal U(1) B L model from dark matter observations
Constraining minimal U(1) B L model from dark matter observations Tanushree Basak Physical Research Laboratory, India 10th PATRAS Workshop on Axions, WIMPs and WISPs CERN Geneva, Switzerland July 3, 2014
More informationA model of the basic interactions between elementary particles is defined by the following three ingredients:
I. THE STANDARD MODEL A model of the basic interactions between elementary particles is defined by the following three ingredients:. The symmetries of the Lagrangian; 2. The representations of fermions
More informationSterile Neutrinos from the Top Down
Sterile Neutrinos from the Top Down Active-sterile mixing The landscape Small Dirac or Majorana masses (or both) The mini-seesaw Light Sterile Neutrinos: A White Paper (K. Abazajian et al), 1204.5379 Neutrino
More informationOn Minimal Models with Light Sterile Neutrinos
On Minimal Models with Light Sterile Neutrinos Pilar Hernández University of Valencia/IFIC Donini, López-Pavón, PH, Maltoni arxiv:1106.0064 Donini, López-Pavón, PH, Maltoni, Schwetz arxiv:1205.5230 SM
More informationNon-Abelian SU(2) H and Two-Higgs Doublets
Non-Abelian SU(2) H and Two-Higgs Doublets Technische Universität Dortmund Wei- Chih Huang 25 Sept 2015 Kavli IPMU arxiv:1510.xxxx(?) with Yue-Lin Sming Tsai, Tzu-Chiang Yuan Plea Please do not take any
More informationNeutrinos and Fundamental Symmetries: L, CP, and CP T
Neutrinos and Fundamental Symmetries: L, CP, and CP T Outstanding issues Lepton number (L) CP violation CP T violation Outstanding issues in neutrino intrinsic properties Scale of underlying physics? (string,
More informationTeV-scale type-i+ii seesaw mechanism and its collider signatures at the LHC
TeV-scale type-i+ii seesaw mechanism and its collider signatures at the LHC Wei Chao (IHEP) Outline Brief overview of neutrino mass models. Introduction to a TeV-scale type-i+ii seesaw model. EW precision
More informationChern-Simons portal Dark Matter
Chern-Simons portal Dark Matter III Saha Theory Workshop: Aspects of Early Universe Cosmology Mathias Pierre Laboratoire de Physique Théorique d Orsay In collaboration with G. Arcadi, G.Bhattacharyya,
More informationNeutrino masses respecting string constraints
Neutrino masses respecting string constraints Introduction Neutrino preliminaries The GUT seesaw Neutrinos in string constructions The triplet model (Work in progress, in collaboration with J. Giedt, G.
More informationSterile Neutrinos in July 2010
Sterile Neutrinos in July 0 Carlo Giunti INFN, Sezione di Torino Presidenza INFN, Roma, 19 July 0 Collaboration with Marco Laveder (Padova University) C. Giunti Sterile Neutrinos in July 0 Presidenza INFN,
More informationkev sterile Neutrino Dark Matter in Extensions of the Standard Model
kev sterile Neutrino Dark Matter in Extensions of the Standard Model Manfred Lindner Max-Planck-Institut für Kernphysik, Heidelberg F. Bezrukov, H. Hettmannsperger, ML, arxiv:0912.4415, PRD81,085032 The
More informationThe Standard Model of particle physics and beyond
The Standard Model of particle physics and beyond - Lecture 3: Beyond the Standard Model Avelino Vicente IFIC CSIC / U. Valencia Physics and astrophysics of cosmic rays in space Milano September 2016 1
More informationKaluza-Klein Theories - basic idea. Fig. from B. Greene, 00
Kaluza-Klein Theories - basic idea Fig. from B. Greene, 00 Kaluza-Klein Theories - basic idea mued mass spectrum Figure 3.2: (Taken from [46]). The full spectrum of the UED model at the first KK level,
More informationDebasish Borah. (Based on with A. Dasgupta)
& Observable LNV with Predominantly Dirac Nature of Active Neutrinos Debasish Borah IIT Guwahati (Based on 1609.04236 with A. Dasgupta) 1 / 44 Outline 1 2 3 4 2 / 44 Evidence of Dark Matter In 1932, Oort
More informationKaluza-Klein Dark Matter
Kaluza-Klein Dark Matter Hsin-Chia Cheng UC Davis Pre-SUSY06 Workshop Complementary between Dark Matter Searches and Collider Experiments Introduction Dark matter is the best evidence for physics beyond
More informationSterile Neutrinos as Dark Matter. Manfred Lindner
Sterile Neutrinos as Dark Matter Manfred Lindner 13-20 December 2012 SM works perfectly & Higgs seems to be there - mass range was shrinking and is now rather precisely known - no signs for anything else
More informationNeutrinos: status, models, string theory expectations
Neutrinos: status, models, string theory expectations Introduction Neutrino preliminaries and status Models String embeddings Intersecting brane The Z 3 heterotic orbifold Embedding the Higgs triplet Outlook
More informationSterile Neutrinos from the Top Down
Sterile Neutrinos from the Top Down Active-sterile mixing The landscape Small Dirac/Majorana masses The mini-seesaw Light Sterile Neutrinos: A White Paper (K. Abazajian et al), 1204.5379 Neutrino Masses
More informationDARK MATTER. Martti Raidal NICPB & University of Helsinki Tvärminne summer school 1
DARK MATTER Martti Raidal NICPB & University of Helsinki 28.05.2010 Tvärminne summer school 1 Energy budget of the Universe 73,4% - Dark Energy WMAP fits to the ΛCDM model Distant supernova 23% - Dark
More informationSterile neutrinos. Stéphane Lavignac (IPhT Saclay)
Sterile neutrinos Stéphane Lavignac (IPhT Saclay) introduction active-sterile mixing and oscillations cosmological constraints experimental situation and fits implications for beta and double beta decays
More informationDark Radiation and Inflationary Freedom
Dark Radiation and Inflationary Freedom Based on [SG et al., JCAP 1504 (2015) 023] [Di Valentino et al., PRD 91 (2015) 123505] Stefano Gariazzo University of Torino, INFN of Torino http://personalpages.to.infn.it/~gariazzo/
More informationLeptogenesis in Higgs triplet model
Leptogenesis in Higgs triplet model S. Scopel Korea Institute of Advanced Study (KIAS) Seoul (Korea) Dark Side of the Universe, Madrid,, 20-24 24 June 2006 Introduction Non-zero neutrino masses and mixing
More informationLeaving Plato s Cave: Beyond The Simplest Models of Dark Matter
Leaving Plato s Cave: Beyond The Simplest Models of Dark Matter Alexander Natale Korea Institute for Advanced Study Nucl. Phys. B914 201-219 (2017), arxiv:1608.06999. High1 2017 February 9th, 2017 1/30
More informationMinimal Extension of the Standard Model of Particle Physics. Dmitry Gorbunov
Minimal Extension of the Standard Model of Particle Physics Dmitry Gorbunov Institute for Nuclear Research, Moscow, Russia 14th Lomonosov Conference on Elementary Paticle Physics, Moscow, MSU, 21.08.2009
More informationYang-Hwan, Ahn (KIAS)
Yang-Hwan, Ahn (KIAS) Collaboration with Paolo Gondolo (Univ. of Utah) Appear to 1312.xxxxx 2013 Particle Theory Group @ Yonsei Univ. 1 The SM as an effective theory Several theoretical arguments (inclusion
More informationA realistic model for DM interactions in the neutrino portal paradigm
A realistic model for DM interactions in the neutrino portal paradigm José I Illana + Vannia González Macías, José Wudka (UC Riverside) 1 Model 2 Constraints 3 Conclusions JHEP 05 (2016) 171 [160105051]
More informationFERMION PORTAL DARK MATTER
FERMION PORTAL DARK MATTER Joshua Berger SLAC UC Davis Theory Seminar! w/ Yang Bai: 1308.0612, 1402.6696 March 10, 2014 1 A HOLE IN THE SM Van Albada et. al. Chandra + Hubble What else can we learn about
More informationMarch 30, 01 Lecture 5 of 6 @ ORICL Philosophical Society Yuri Kamyshkov/ University of Tennessee email: kamyshkov@utk.edu 1. Concept/misconception of mass in Special Relativity (March,9). and n Oscillations:
More informationBeyond the Standard Model
Beyond the Standard Model The Standard Model Problems with the Standard Model New Physics Supersymmetry Extended Electroweak Symmetry Grand Unification References: 2008 TASI lectures: arxiv:0901.0241 [hep-ph]
More informationCosmological Constraint on the Minimal Universal Extra Dimension Model
Cosmological Constraint on the Minimal Universal Extra Dimension Model Mitsuru Kakizaki (Bonn University) September 7, 2007 @ KIAS In collaboration with Shigeki Matsumoto (Tohoku Univ.) Yoshio Sato (Saitama
More informationDark matter and entropy dilution
Dark matter and entropy dilution Miha Nemevšek Goran Senjanović, Yue Zhang 1205.0844 Dark workshop TÜM/IAS, December 2015 Dark Matter stability Discrete symmetries MSSM & R-parity extended Higgs Inert
More informationModels of New Physics for Dark Matter
Models of New Physics for Dark Matter Carlos Muñoz instituto de física teórica ift-uam/csic departamento de física teórica dft-uam 1 PPC 2010, Torino, July 12-16 Crucial Moment for SUSY in next few years:
More informationProbing the Majorana nature in radiative seesaw models at collider experiments
Probing the Majorana nature in radiative seesaw models at collider experiments Shinya KANEMURA (U. of Toyama) M. Aoki, SK and O. Seto, PRL 102, 051805 (2009). M. Aoki, SK and O. Seto, PRD80, 033007 (2009).
More informationEffective Theory for Electroweak Doublet Dark Matter
Effective Theory for Electroweak Doublet Dark Matter University of Ioannina, Greece 3/9/2016 In collaboration with Athanasios Dedes and Vassilis Spanos ArXiv:1607.05040 [submitted to PhysRevD] Why dark
More informationNeutrino Mass in Strings
Neutrino Mass in Strings Introduction Neutrino preliminaries Models String embeddings Intersecting brane The Z 3 heterotic orbifold Embedding the Higgs triplet Outlook Neutrino mass Nonzero mass may be
More informationModels of Neutrino Masses
Models of Neutrino Masses Fernando Romero López 13.05.2016 1 Introduction and Motivation 3 2 Dirac and Majorana Spinors 4 3 SU(2) L U(1) Y Extensions 11 4 Neutrino masses in R-Parity Violating Supersymmetry
More informationNeutrino Oscillation, Leptogenesis and Spontaneous CP Violation
Neutrino Oscillation, Leptogenesis and Spontaneous CP Violation Mu-Chun Chen Fermilab (Jan 1, 27: UC Irvine) M.-C. C & K.T. Mahanthappa, hep-ph/69288, to appear in Phys. Rev. D; Phys. Rev. D71, 351 (25)
More informationDark matter and IceCube neutrinos
IL NUOVO CIMENTO 38 C (2015) 31 DOI 10.1393/ncc/i2015-15031-4 Colloquia: IFAE 2014 Dark matter and IceCube neutrinos R. Biondi Dipartimento di Scienze Fisiche e Chimiche, Università degli Studi di L Aquila,
More informationThe Physics of Heavy Z-prime Gauge Bosons
The Physics of Heavy Z-prime Gauge Bosons Tevatron LHC LHC LC LC 15fb -1 100fb -1 14TeV 1ab -1 14TeV 0.5TeV 1ab -1 P - =0.8 P + =0.6 0.8TeV 1ab -1 P - =0.8 P + =0.6 χ ψ η LR SSM 0 2 4 6 8 10 12 2σ m Z'
More informationRight-Handed Neutrinos as the Origin of the Electroweak Scale
Right-Handed Neutrinos as the Origin of the Electroweak Scale Hooman Davoudiasl HET Group, Brookhaven National Laboratory Based on: H. D., I. Lewis, arxiv:1404.6260 [hep-ph] Origin of Mass 2014, CP 3 Origins,
More informationDark Matter and Gauged Baryon Number
Dark Matter and Gauged Baryon Number Sebastian Ohmer Collaborators: Pavel Fileviez Pérez and Hiren H. Patel P. Fileviez Pérez, SO, H. H. Patel, Phys.Lett.B735(2014)[arXiv:1403.8029] P.Fileviez Pérez, SO,
More informationInvisible Sterile Neutrinos
Invisible Sterile Neutrinos March 25, 2010 Outline Overview of Sterile Neutrino Dark Matter The Inert Doublet Model with 3 Singlet Fermions Non-thermal Dark Matter Conclusion Work done in collaboration
More informationStatus and prospects of neutrino oscillations
Status and prospects of neutrino oscillations S. Bilenky JINR(Dubna)TRIUMF June 10, 2017 The award of the 2015 Nobel Prize to T. Kajita and A. McDonald for the discovery of neutrino oscillations, which
More informationYang-Hwan, Ahn (KIAS)
Yang-Hwan, Ahn (KIAS) Collaboration with Paolo Gondolo (Univ. of Utah) Appear to 1311.xxxxx The 3 rd KIAS workshop on Particle physics and Cosmology 1 The SM as an effective theory Several theoretical
More informationLeptogenesis. Neutrino 08 Christchurch, New Zealand 30/5/2008
Leptogenesis Neutrino 08 Christchurch, New Zealand 30/5/2008 Yossi Nir (Weizmann Institute of Science) Sacha Davidson, Enrico Nardi, YN Physics Reports, in press [arxiv:0802.2962] E. Roulet, G. Engelhard,
More informationElectroweak-scale Right-handed Neutrino Model And 126 GeV Higgs-like Particle
Electroweak-scale Right-handed Neutrino Model And 126 GeV Higgs-like Particle Ajinkya S. Kamat ask4db@virginia.edu http://people.virginia.edu/ ask4db With Prof. P. Q. Hung and Vinh Van Hoang (paper in
More informationTechnicolor Dark Matter. Chris Kouvaris Université Libre de Bruxelles
Technicolor Dark Matter Chris Kouvaris Université Libre de Bruxelles Dynamical Symmetry breaking: The motivation for Technicolor Long time before QCD BCS showed that the Fermi surfaces are unstable to
More informationU(1) Gauge Extensions of the Standard Model
U(1) Gauge Extensions of the Standard Model Ernest Ma Physics and Astronomy Department University of California Riverside, CA 92521, USA U(1) Gauge Extensions of the Standard Model (int08) back to start
More informationFermionic DM Higgs Portal! An EFT approach
Fermionic DM Higgs Portal An EFT approach Michael A. Fedderke University of Chicago Based on 1404.83 [hep-ph] (MF, Chen, Kolb, Wang) Unlocking the Higgs Portal ACFI, UMass, Amherst May 014 01 discovery
More informationBaryon-Lepton Duplicity as the Progenitor of Long-Lived Dark Matter
UCRHEP-T593 Aug 018 arxiv:1808.05417v [hep-ph] 5 Jan 019 Baryon-Lepton Duplicity as the Progenitor of Long-Lived Dark Matter Ernest Ma Physics and Astronomy Department, University of California, Riverside,
More informationPhenomenology of low-energy flavour models: rare processes and dark matter
IPMU February 2 nd 2016 Phenomenology of low-energy flavour models: rare processes and dark matter Lorenzo Calibbi ITP CAS, Beijing Introduction Why are we interested in Flavour Physics? SM flavour puzzle
More informationSplit Supersymmetry A Model Building Approach
Split Supersymmetry A Model Building Approach Kai Wang Phenomenology Institute Department of Physics the University of Wisconsin Madison UC Riverside HEP Seminar In Collaboration with Ilia Gogoladze (Notre
More informationNeutrino Mass Models
Neutrino Mass Models S Uma Sankar Department of Physics Indian Institute of Technology Bombay Mumbai, India S. Uma Sankar (IITB) IWAAP-17, BARC (Mumbai) 01 December 2017 1 / 15 Neutrino Masses LEP experiments
More informationTwo hot issues in neutrino physics
Bari Xmas Workshop /1/011 Two hot issues in neutrino physics Antonio Palazzo Excellence Cluster Universe - TUM 1 Outline! - Introduction - The evidence of! 13 >0 - Hints of new light sterile neutrinos
More informationGALACTIC CENTER GEV GAMMA- RAY EXCESS FROM DARK MATTER WITH GAUGED LEPTON NUMBERS. Jongkuk Kim (SKKU) Based on Physics Letters B.
GALACTIC CENTER GEV GAMMA- RAY EXCESS FROM DARK MATTER WITH GAUGED LEPTON NUMBERS Jongkuk Kim (SKKU) Based on Physics Letters B. 752 (2016) 59-65 In collaboration with Jong Chul Park, Seong Chan Park The
More informationNeutrino Oscillations And Sterile Neutrinos
Neutrino Oscillations And Sterile Neutrinos Keshava Prasad Gubbi University of Bonn s6nagubb@uni-bonn.de May 27, 2016 Keshava Prasad Gubbi (Uni Bonn) Neutrino Oscillations,Sterile Neutrinos May 27, 2016
More informationPossible sources of very energetic neutrinos. Active Galactic Nuclei
Possible sources of very energetic neutrinos Active Galactic Nuclei 1 What might we learn from astrophysical neutrinos? Neutrinos not attenuated/absorbed Information about central engines of astrophysical
More informationPhysics at e + e - Linear Colliders. 4. Supersymmetric particles. M. E. Peskin March, 2002
Physics at e + e - Linear Colliders 4. Supersymmetric particles M. E. Peskin March, 2002 In this final lecture, I would like to discuss supersymmetry at the LC. Supersymmetry is not a part of the Standard
More informationSupersymmetry Breaking
Supersymmetry Breaking LHC Search of SUSY: Part II Kai Wang Phenomenology Institute Department of Physics University of Wisconsin Madison Collider Phemonology Gauge Hierarchy and Low Energy SUSY Gauge
More informationRelating the Baryon Asymmetry to WIMP Miracle Dark Matter
Brussels 20/4/12 Relating the Baryon Asymmetry to WIMP Miracle Dark Matter PRD 84 (2011) 103514 (arxiv:1108.4653) + PRD 83 (2011) 083509 (arxiv:1009.3227) John McDonald, LMS Consortium for Fundamental
More informationThe Yang and Yin of Neutrinos
The Yang and Yin of Neutrinos Ernest Ma Physics and Astronomy Department University of California Riverside, CA 92521, USA The Yang and Yin of Neutrinos (2018) back to start 1 Contents Introduction The
More informationThe Stueckelberg Extension and Extra Weak Dark Matter
The Stueckelberg Extension and Extra Weak Dark Matter PN Miami-2006 Conference with Boris Kors, Daniel Feldman, and Zuowei Liu CDM Candidates Axion Right handed neutrino Neutralino Singlino Sneutrino KK
More informationComputer tools in particle physics
Computer tools in particle physics - Lecture 1 : SARAH and SPheno - Avelino Vicente IFIC CSIC / U. Valencia Curso de doctorado de la U. València IFIC February 1-5 2016 Avelino Vicente - Computer tools
More informationACCIDENTAL DARK MATTER: A CASE IN SCALE INVARIANT B-L MODEL
THE 4TH KIAS WORKSHOP ON PARTICLE PHYSICS AND COSMOLOGY ACCIDENTAL DARK MATTER: A CASE IN SCALE INVARIANT B-L MODEL ZHAOFENG KANG, KIAS, SEOUL, 10/31/2014 BASED ON AN UNBORN PAPER, WITH P. KO, Y. ORIKAS
More informationFlavor Physics in the multi-higgs doublet models induced by the left-right symmetry
Flavor Physics in the multi-higgs doublet models induced by the left-right symmetry Yoshihiro Shigekami KEK HUST ( 華中科技大学 ), Wuhan ( 武漢 ) Syuhei Iguro (Nagoya U.), Yu Muramatsu (CCNU), Yuji Omura (Nagoya
More informationSymmetry Origin of Observable Nonunitary Neutrino Mixng Matrix in TeV Scale Seesaw Models
Symmetry Origin of Observable Nonunitary Neutrino Mixng Matrix in TeV Scale Seesaw Models Ernest Ma Physics and Astronomy Department University of California Riverside, CA 92521, USA Symmetry Origin of
More informationNon-zero Ue3, Leptogenesis in A4 Symmetry
Non-zero Ue3, Leptogenesis in A4 Symmetry 2 nd International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry Y.H.Ahn (Academia Sinica) based on the paper with C.S.Kim and S. Oh 1 Outline
More informationDark matter and collider signatures from extra dimensions
KAIST TF, A. Menon, Z. Sullivan, PRD 86 (2012) 093006 L. Edelhäuser, TF, M. Krämer, JHEP 1308 (2013) 091 TF, KC Kong, SC Park, JHEP 1305 (2013) 111, arxiv:1309.xxxx COSMO 2013, Cambridge Outline Universal
More informationThe Higgs Mechanism and the Higgs Particle
The Higgs Mechanism and the Higgs Particle Heavy-Ion Seminar... or the Anderson-Higgs-Brout-Englert-Guralnik-Hagen-Kibble Mechanism Philip W. Anderson Peter W. Higgs Tom W. B. Gerald Carl R. François Robert
More informationParticle Physics: Neutrinos part II
Particle Physics: Neutrinos part II José I. Crespo-Anadón Week 9: April 1, 2017 Columbia University Science Honors Program Course Policies Attendance Up to four absences Send email notifications of all
More informationHow many neutrino species are there?
How many neutrino species are there? Jan Hamann 6. Kosmologietag, Bielefeld 5-6 May 2011 Radiation content of the Universe Microwave background Neutrino background standard model expectation: [Mangano
More informationLittle Higgs Models Theory & Phenomenology
Little Higgs Models Theory Phenomenology Wolfgang Kilian (Karlsruhe) Karlsruhe January 2003 How to make a light Higgs (without SUSY) Minimal models The Littlest Higgs and the Minimal Moose Phenomenology
More informationNeutrinos secretly converting to lighter particles to please both KATRIN and Cosmos. Yasaman Farzan IPM, Tehran
Neutrinos secretly converting to lighter particles to please both KATRIN and Cosmos Yasaman Farzan IPM, Tehran Outline Motivation for the KATRIN experiment Effect of neutrinos on cosmological scales and
More informationThe Flavour Portal to Dark Matter
Dark Side of the Universe 2015 Kyoto University The Flavour Portal to Dark Matter Lorenzo Calibbi ITP CAS, Beijing December 18th 2015 Introduction Why are we interested in Flavour Physics? SM flavour puzzle
More informationGauge U(1) Dark Symmetry and Radiative Light Fermion Masses
UCRHEP-T565 April 2016 arxiv:1604.01148v1 [hep-ph] 5 Apr 2016 Gauge U(1) Dark Symmetry and Radiative Light Fermion Masses Corey Kownacki 1 and Ernest Ma 1,2,3 1 Department of Physics and Astronomy, University
More informationWIMPs and superwimps. Jonathan Feng UC Irvine. MIT Particle Theory Seminar 17 March 2003
WIMPs and superwimps Jonathan Feng UC Irvine MIT Particle Theory Seminar 17 March 2003 Dark Matter The dawn (mid-morning?) of precision cosmology: Ω DM = 0.23 ± 0.04 Ω total = 1.02 ± 0.02 Ω baryon = 0.044
More informationUpdating the Status of Neutrino Physics
Updating the Status of Neutrino Physics J. W. F. Valle IFIC-CSIC/U. Valencia Based on hep-ph/36 and hep-ph/3792 String Phenomenology 23, Durham p. Atmospheric zenith distribution Maltoni, Schwetz, Tortola
More informationLeft-Right Symmetric Models with Peccei-Quinn Symmetry
Left-Right Symmetric Models with Peccei-Quinn Symmetry Pei-Hong Gu Max-Planck-Institut für Kernphysik, Heidelberg PHG, 0.2380; PHG, Manfred Lindner, 0.4905. Institute of Theoretical Physics, Chinese Academy
More informationSUPERSYMETRY FOR ASTROPHYSICISTS
Dark Matter: From the Cosmos to the Laboratory SUPERSYMETRY FOR ASTROPHYSICISTS Jonathan Feng University of California, Irvine 29 Jul 1 Aug 2007 SLAC Summer Institute 30 Jul 1 Aug 07 Feng 1 Graphic: N.
More informationGauged U(1) clockwork
Gauged U(1) clockwork Hyun Min Lee Chung-Ang University, Korea Based on arxiv: 1708.03564 Workshop on the Standard Model and Beyond Corfu, Greece, Sept 2-10, 2017. Outline Introduction & motivation Gauged
More informationNeutrinos. Riazuddin National Centre for Physics Quaid-i-Azam University Campus. Islamabad.
Neutrinos Riazuddin National Centre for Physics Quaid-i-Azam University Campus Islamabad. Neutrino was the first particle postulated by a theoretician: W. Pauli in 1930 to save conservation of energy and
More informationSterile Neutrinos in Cosmology and Astrophysics
Kalliopi Petraki (UCLA) October 27, 2008 Particle Physics Neutrino Oscillation experiments: neutrinos have mass Cosmology and Astrophysics Plenty of unexplained phenomena Dark Matter Pulsar Kicks Supernova
More informationBeyond Simplified Models
Pseudoscalar Portal to Dark Matter: Beyond Simplified Models Jose Miguel No King's College London J.M.N. PRD 93 (RC) 031701 (1509.01110) D. Goncalves, P. Machado, J.M.N. 1611.04593 M. Fairbairn, J.M.N.,
More informationarxiv: v2 [hep-ph] 5 Dec 2017
Common Origin of 3.55 kev X-ray line and Gauge Coupling Unification with Left-ight Dark Matter arxiv:1604.0199v [hep-ph] 5 Dec 017 Debasish Borah, 1, Arnab Dasgupta,, 3, 4, 5, and Sudhanwa Patra 1 Department
More informationMirror fermions, electroweak scale right-handed neutrinos and experimental implications
Mirror fermions, electroweak scale right-handed neutrinos and experimental implications P. Q. Hung University of Virginia Ljubljana 2008 Plan of Talk The question of parity restoration at high energies:
More informationZ -portal right-handed neutrino dark ma4er in the minimal U(1)x extended Standard Model
Z -portal right-handed neutrino dark ma4er in the minimal U(1)x extended Standard Model Nobuchika Okada University of Alabama In collaborapon with Satomi Okada (Yamagata Univ., Japan) Ref: NO & S. Okada,
More informationLecture 03. The Standard Model of Particle Physics. Part III Extensions of the Standard Model
Lecture 03 The Standard Model of Particle Physics Part III Extensions of the Standard Model Where the SM Works Excellent description of 3 of the 4 fundamental forces Explains nuclear structure, quark confinement,
More informationNew Physics from the String Vacuum
New Physics from the String Vacuum The string vacuum Extended MSSM quivers String remnants Small neutrino masses Quivers: Cvetič, Halverson, PL, JHEP 1111,058 (1108.5187) Z : Rev.Mod.Phys.81,1199 (0801.145)
More informationGeV neutrino mass models: Experimental reach vs. theoretical predictions RWR, Walter Winter Arxiv PRD 94, (2016)
GeV neutrino mass models: Experimental reach vs. theoretical predictions RWR, Walter Winter Arxiv 1607.07880 PRD 94, 073004 (016) Rasmus W. Rasmussen Matter and the Universe 1-1-16 Theory of elementary
More informationStefano Gariazzo. Light sterile neutrinos with pseudoscalar interactions in cosmology. Based on [JCAP 08 (2016) 067] University and INFN, Torino
Stefano Gariazzo University and INFN, Torino gariazzo@to.infn.it http://personalpages.to.infn.it/~gariazzo/ Light sterile neutrinos with pseudoscalar interactions in cosmology Based on [JCAP 08 (2016)
More informationHow high could SUSY go?
How high could SUSY go? Luc Darmé LPTHE (Paris), UPMC November 24, 2015 Based on works realised in collaboration with K. Benakli, M. Goodsell and P. Slavich (1312.5220, 1508.02534 and 1511.02044) Introduction
More informationPhysics beyond the Standard Model: Neutrinos & Dark matter
Physics beyond the Standard Model: Neutrinos & Dark matter José W F Valle http://astroparticles.ific.uv.es/ PASCOS 2013, Taiwan 1 Where do neutrinos come from? 336 / cm3: bilions of Cosmic neutrinos Cross
More information