CTP Approach to Leptogenesis
|
|
- Sherilyn Weaver
- 6 years ago
- Views:
Transcription
1 CTP Approach to Leptogenesis Matti Herranen a in collaboration with Martin Beneke a Björn Garbrecht a Pedro Schwaller b Institut für Theoretische Teilchenphysik und Kosmologie, RWTH Aachen University a Institut für Theoretische Physik, Universität Zürich b 5. Kosmologietag, Bielefeld, M. Herranen (RWTH Aachen) Bielefeld, / 22
2 Outline Introduction Standard Approach to Leptogenesis Closed Time Path (CTP) Approach to Leptogenesis Conclusions and outlook M. Herranen (RWTH Aachen) Bielefeld, / 22
3 Why baryogenesis? to explain the excess of matter over antimatter in the universe: [WMAP 2003] n B = ( ) n γ Challenge: Inflation washes out any initial baryon number. Some dynamical mechanism = baryogenesis is needed M. Herranen (RWTH Aachen) Bielefeld, / 22
4 Leptogenesis [Fukugita, Yanagida (1986)] The Standard Model is extended by adding heavy right-handed Majorana neutrinos N i, i = 1, 2,... (eg. see-saw models) L h β (l βφ) e Rβ Y αk(l α φ ) N k 1 2 N jm j N c j + h.c. M. Herranen (RWTH Aachen) Bielefeld, / 22
5 Leptogenesis [Fukugita, Yanagida (1986)] The Standard Model is extended by adding heavy right-handed Majorana neutrinos N i, i = 1, 2,... (eg. see-saw models) L h β (l βφ) e Rβ Y αk(l α φ ) N k 1 2 N jm j N c j + h.c. Key element: out-of-equilibrium L- and CP-violating Yukawa decays of the heavy Majorana neutrinos ε 1 Γ(N1 lφ) Γ(N1 lφ ) Γ(N 1 lφ) + Γ(N 1 lφ ) 1 X M 1 Im ([Y Y] 2 1j) 8π M j [Y Y] 11 j M. Herranen (RWTH Aachen) Bielefeld, / 22
6 Baryogenesis via Leptogenesis The Sakharov conditions (1967) must be fulfilled: Baryon number B violation C violation CP violation Out of equilibrium M. Herranen (RWTH Aachen) Bielefeld, / 22
7 Baryogenesis via Leptogenesis The Sakharov conditions (1967) must be fulfilled: Baryon number B violation B L broken by neutrino Majorana masses B + L broken by the electroweak Sphalerons C violation Left-chiral electroweak interactions CP violation Yukawa interactions between the charged leptons l α and the Majorana neutrinos N i Out of equilibrium Expansion of the Universe - decreasing temperature T Heavy neutrino decays become out of equilibrium when M 1 T M. Herranen (RWTH Aachen) Bielefeld, / 22
8 2. Standard Approach to Leptogenesis M. Herranen (RWTH Aachen) Bielefeld, / 22
9 Boltzmann Equations for Leptogenesis (n l n l ) + 3H(n l n l ) t d 3 k = (2π) 3 2 d 3 p d 3 q k 2 + Mi 2 (2π) 3 2 p (2π) 3 2 q (2π)4 δ 4 (k p q) { M N1 lφ 2 f Ni (k) M N1 lφ 2 f Ni (k) } M lφ N1 2 f l (p)f φ (q) + M lφ N1 2 f l(p)f φ (q) d 3 k d 3 l d 3 p d 3 q + (2π) 3 2 k (2π) 3 2 l (2π) 3 2 p (2π) 3 2 q (2π)4 δ 4 (k + l p q) { } M lφ lφ 2 f l(k))f φ (l) M lφ lφ 2 f l (k))f φ (l) Expressed in terms of vacuum matrix elements M α β M. Herranen (RWTH Aachen) Bielefeld, / 22
10 Vacuum Matrix Elements and RIS Subtraction Naive multiplication suggests asymmetry even in equilibrium: Γ lφ lφ 1 + 2ε The on-shell intermediate states of 2 2 processes are already accounted for by the 1 2 Real Intermediate State subtraction is needed M. Herranen (RWTH Aachen) Bielefeld, / 22
11 4. CTP Approach to Leptogenesis 1 1 related / complementary aspects in: Buchmüller, Fredenhagen (2000); De Simone, Riotto (2007); Garny, Hohenegger, Kartavtsev, Lindner (2009 & 2010); Anisimov, Buchmüller, Drewes, Mendizabal (2010) M. Herranen (RWTH Aachen) Bielefeld, / 22
12 Closed Time Path (CTP) Formalism a.k.a. Schwinger-Keldysh Formalism [Schwinger (1961); Keldysh (1964); Calzetta, Hu (1988)] In the heuristic Boltzmann equations, matrix elements are computed within the usual in-out framework: out S in time-ordered correlators: T[ψ(x) ψ(y)] In leptogenesis we want to calculate expectation values, e.g. charge density: j 0 (x) = ψ(x)γ 0 ψ(x), in a finite density medium M. Herranen (RWTH Aachen) Bielefeld, / 22
13 Closed Time Path (CTP) Formalism a.k.a. Schwinger-Keldysh Formalism [Schwinger (1961); Keldysh (1964); Calzetta, Hu (1988)] In the heuristic Boltzmann equations, matrix elements are computed within the usual in-out framework: out S in time-ordered correlators: T[ψ(x) ψ(y)] In leptogenesis we want to calculate expectation values, e.g. charge density: j 0 (x) = ψ(x)γ 0 ψ(x), in a finite density medium In-In generating functional on a Closed Time Path: Im t Path-ordered correlators: Re t ig C (x, y) = T C [ψ(x) ψ(y)] M. Herranen (RWTH Aachen) Bielefeld, / 22
14 Four propagators with respect to real time variable: ig + (u, v) = ig < (u, v) = ψ(v)ψ(u) ig + (u, v) = ig > (u, v) = ψ(u) ψ(v) ig ++ (u, v) = ig T (u, v) = T(ψ(u) ψ(v)) ig (u, v) = ig T (u, v) = T(ψ(u) ψ(v)) Free propagators in momentum space: ig < (p) = 2πδ(p 2 m 2 )(p/ + m) ˆϑ(p 0)f (p) ϑ( p 0)(1 f ( p)) ig > (p) = 2πδ(p 2 m 2 )(p/ + m) ˆ ϑ(p 0)(1 f (p)) + ϑ( p 0) f ( p) ig T i(p/ + m) (p) = p 2 m 2 + iε 2πδ(p2 m 2 )(p/ + m) ˆϑ(p 0)f (p) + ϑ( p 0) f ( p) ig T i(p/ + m) (p) = p 2 m 2 iε 2πδ(p2 m 2 )(p/ + m) ˆϑ(p 0)f (p) + ϑ( p 0) f ( p) f (p) and f (p) are the distribution functions of particles and antiparticles M. Herranen (RWTH Aachen) Bielefeld, / 22
15 Kadanoff-Baym Equations Schwinger-Dyson equations for (CTP) propagators: G G 0 = + Σ The Kadanoff-Baym equations are the <, > components: (i / m)g <,> Σ H G <,> Σ <,> G H = 1 ( Σ > G < Σ < G >) 2 M. Herranen (RWTH Aachen) Bielefeld, / 22
16 Kadanoff-Baym Equations Schwinger-Dyson equations for (CTP) propagators: G G 0 = + Σ The Kadanoff-Baym equations are the <, > components: (i / m)g <,> Σ H G <,> Σ <,> G H = 1 ( Σ > G < Σ < G >) 2 Approximations: Wigner transformation: G(k, x) = d 4 r e ik r G(x + r 2, x r 2 ), and gradient expansion to the lowest order (also in finite width Γ) The propagators are reduced to the free theory form Kinetic equations describe the evolution of f (p, t) and f (p, t): d dt γ 0iG <,> (k) = [ iσ > (k)ig < (k) iσ < (k)ig > (k) ] M. Herranen (RWTH Aachen) Bielefeld, / 22
17 Tree-Level Collision Terms in (Unflavoured) Leptogenesis The leading order self energies: l: N: iσ ab l (k) = Y i 2 d 4 k (2π) 4 d 4 k (2π) 4 (2π)4 δ (4) (k k k )P R ig ab Ni(k )P L i ba φ ( k ) d iσ ab 4 k d 4 k { Nij(k) = g w (2π) 4 (2π) 4 (2π)4 δ (4) (k k k ) Y i Yj P L ig ab l (k )P R i ab φ (k ) + Y i Y j C [ P L ig ba l ( k )P R ] T C i ba φ ( k ) } M. Herranen (RWTH Aachen) Bielefeld, / 22
18 Kinetic Equation for Lepton Asymmetry d dt (n l n l ) = d dt = d 4 k (2π) 4 γ 0iG <,> (k) d 4 k [ iσ > (2π) 4 (k)ig < (k) iσ < (k)ig > (k) ] = Y i 2 d 3 k d 3 k (2π) 3 2 k 2 (2π) 3 2 d 3 k k 2 + Mi 2 (2π) 3 2 k { (2π) 4 δ 4 (k k k ) 2k k (1 f Ni (k )) [f l (k)f φ (k ) f l (k) f φ (k )] } f Ni (k ) [(1 f l (k))(1 + f φ (k )) (1 f l (k))(1 + f φ (k ))] Washout contribution M. Herranen (RWTH Aachen) Bielefeld, / 22
19 KMS Relations [Kubo (1957); Martin, Schwinger (1959)] A useful symmetry for correlators in thermal equilibrium: ig > l,n (p) = eβp 0 ig < l,n (p), i > φ (p) = eβp 0 i < φ (p) Hold for (thermal) self energies as well: iσ > l,n (p) = eβp 0 iσ < l,n (p), iπ> φ (p) = eβp 0 iπ < φ (p) KMS relations imply the vanishing of the collision term in thermal equilibrium: iσ > (k)ig < (k) iσ < (k)ig > (k) = 0 }{{} ( e βp 0 iσ > (p))( e βp 0 ig < (p)) Within the CTP formalism, we get the vanishing of the asymmetry in equilibrium for free M. Herranen (RWTH Aachen) Bielefeld, / 22
20 Wave-function Contribution Orange cut Interference between two s-channel scatterings Blue cut Interference between loop and tree-level decays Z d 3 k (2π) 3 Cwf l (k) = 4 Im[Y1 2 Y2 2 ] Z M 1M 2 M1 2 M2 2 d 3 k q (2π) 3 2 k 2 + M1 2 δf N(k ) ΣNµ(k )Σ µ N (k ) g w where the thermal decay rate is Z Σ µ d 3 p d 3 q N(k) = g w (2π) 3 2 p (2π) 3 2 q (2π)4 δ 4 (k p q) p µ 1 f eq eq l (p) + fφ (q) When neglecting quantum-statistical corrections (i.e. (1 f l,n ) 1 and (1 + f φ ) 1), we recover the usual RIS M. Herranen (RWTH Aachen) Bielefeld, / 22
21 Vertex Contribution Orange cut Interference between s- and t-channel scatterings Blue cut Interference between loop and tree-level decays Z d 3 p Z (2π) 3 Cv l(p ) = 4 Im[Y1 2 Y2 2 d 3 k ] (2π) 3 2 p δf N1(k) V(k, M 2), k 2 + M1 2 Z d 3 p d 3 p V(k, M 2) = (2π) 3 2 p (2π) 3 2 p (2π)4 δ 4 (k p p ) p µ Γ µ(k, p, M 2) ˆ1 f l (p ) + f φ (p ) Thermal vertex function: Z Γ µ(k, p d 3 k d 3 k, M 2) = (2π) 3 2 k (2π) 3 2 k (2π)4 δ 4 (k k k ) k µ M 1M 2 (k p ) 2 M2 2 ˆ1 f l (k ) + f φ (k ) M. Herranen (RWTH Aachen) Bielefeld, / 22
22 Numerical Results: Effective CP-Violating Parameter Consider limit M 1 M 2 : ε wf eff ε wf T=0 = 16π g w d k k 2 k 0 Σ µ N1 (k)σ N1 µ(k) δf N1 (k) d k k 2 k µ Σ µ N1 (k) δf N1(k) k Ε eff Ε T 0 1 Expect large effect for weak washout small effect for strong washout z M 1 T M. Herranen (RWTH Aachen) Bielefeld, / 22
23 Lepton Asymmetry: Y l = n l n l s, Strong Washout Y l z M 1 T blue: thermal initial f N1 solid: full solution red: zero initial f N1 dashed: no thermal corrections in loops M 1 = GeV, M 2 = GeV, Y 1 = , Y 2 = 10 1, Im[Y 1Y 2 ] = Y 1Y 2 M. Herranen (RWTH Aachen) Bielefeld, / 22
24 Lepton Asymmetry: Y l = n l n l s, Moderate Washout Y l z M 1 T blue: thermal initial f N1 solid: full solution red: zero initial f N1 dashed: no thermal corrections in loops M 1 = GeV, M 2 = GeV, Y 1 = , Y 2 = 10 1, Im[Y 1Y 2 ] = Y 1Y 2 M. Herranen (RWTH Aachen) Bielefeld, / 22
25 Lepton Asymmetry: Y l = n l n l s, Weak Washout Y l z M 1 T blue: thermal initial f N1 solid: full solution red: zero initial f N1 dashed: no thermal corrections in loops M 1 = GeV, M 2 = GeV, Y 1 = , Y 2 = 10 1, Im[Y 1Y 2 ] = Y 1Y 2 M. Herranen (RWTH Aachen) Bielefeld, / 22
26 Conclusion and outlook Conclusions: First principle description of Leptogenesis within the CTP framework Alternative - perhaps more satisfactory - manifestation of CPT invariance in the kinetic equation when compared to the usual RIS subtraction scheme Full inclusion of quantum statistical corrections in loops and external states (contribute at the same level) M. Herranen (RWTH Aachen) Bielefeld, / 22
27 Conclusion and outlook Conclusions: First principle description of Leptogenesis within the CTP framework Alternative - perhaps more satisfactory - manifestation of CPT invariance in the kinetic equation when compared to the usual RIS subtraction scheme Full inclusion of quantum statistical corrections in loops and external states (contribute at the same level) Outlook: Flavor coherence effects, finite width effects, resonant Leptogenesis M. Herranen (RWTH Aachen) Bielefeld, / 22
Recent progress in leptogenesis
XLIII rd Rencontres de Moriond Electroweak Interactions and Unified Theories La Thuile, Italy, March 1-8, 2008 Recent progress in leptogenesis Steve Blanchet Max-Planck-Institut for Physics, Munich March
More informationTTK Coherent quantum Boltzmann equations from cqpa Matti Herranen a, Kimmo Kainulainen b;c and Pyry Matti Rahkila b;c a Institut f ur Theoretisc
TTK-10-34 Coherent quantum Boltzmann equations from cqpa Matti Herranen a, Kimmo Kainulainen b;c and Pyry Matti Rahkila b;c a Institut f ur Theoretische Teilchenphysik und Kosmologie, RWTH Aachen University,
More informationOn the double-counting problem in Boltzmann equations and real-intermediate state subtraction
On the double-counting problem in Boltzmann equations and real-intermediate state subtraction Mcgill University, Nov. 2017 Outline 1 Introduction Baryogenesis 2 History S.Wolfram and E.Kolb (1980) Issues
More informationEffects of Reheating on Leptogenesis
Effects of Reheating on Leptogenesis Florian Hahn-Woernle Max-Planck-Institut für Physik München 2. Kosmologietag Florian Hahn-Woernle (MPI-München) Effects of Reheating on Leptogenesis Kosmologietag 2007
More informationLeptogenesis via varying Weinberg operator
Silvia Pascoli IPPP, Department of Physics, Durham University, Durham DH1 3LE, United Kingdom E-mail: silvia.pascoli@durham.ac.uk Jessica Turner Theoretical Physics Department, Fermi National Accelerator
More informationLeptogenesis from GeV-Scale Sterile Neutrinos
Leptogenesis from GeV-Scale Sterile Neutrinos Björn Garbrecht Physik-Department T70 Technische Universität München Lorentz Center Workshop Matter over Antimatter: The Sakharov conditions After 50 years
More informationA biased review of Leptogenesis. Lotfi Boubekeur ICTP
A biased review of Leptogenesis Lotfi Boubekeur ICTP Baryogenesis: Basics Observation Our Universe is baryon asymmetric. n B s n b n b s 10 11 BAU is measured in CMB and BBN. Perfect agreement with each
More informationEntropy, Baryon Asymmetry and Dark Matter from Heavy Neutrino Decays.
Entropy, Baryon Asymmetry and Dark Matter from Heavy Neutrino Decays. Kai Schmitz Deutsches Elektronen-Synchrotron DESY, Hamburg, Germany Based on arxiv:1008.2355 [hep-ph] and arxiv:1104.2750 [hep-ph].
More informationLeptogenesis. Alejandro Ibarra Technische Universität München. Warsaw February 2010
Leptogenesis Alejandro Ibarra Technische Universität München Warsaw February 2010 Outline Evidence for a baryon asymmetry Sakharov conditions GUT baryogenesis Sphalerons Neutrino masses and its origin
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 informationMatter vs Anti-matter
Baryogenesis Matter vs Anti-matter Earth, Solar system made of baryons B Our Galaxy Anti-matter in cosmic rays p/p O(10 4 ) secondary Our Galaxy is made of baryons p galaxy p + p p + p + p + p galaxy γ
More informationKadanoff-Baym Equations and Baryogenesis
KBE, Kiel, 13.10.11 Nonequilibrium dynamics at high energy Heavy Ion Collisions LHC: ALICE RHIC Early universe Reheating after Inflation Dark matter freeze-out Baryogenesis... Outline Matter-Antimatter
More informationLeptogenesis with Composite Neutrinos
Leptogenesis with Composite Neutrinos Based on arxiv:0811.0871 In collaboration with Yuval Grossman Cornell University Friday Lunch Talk Yuhsin Tsai, Cornell University/CIHEP Leptogenesis with Composite
More informationOverview of mass hierarchy, CP violation and leptogenesis.
Overview of mass hierarchy, CP violation and leptogenesis. (Theory and Phenomenology) Walter Winter DESY International Workshop on Next Generation Nucleon Decay and Neutrino Detectors (NNN 2016) 3-5 November
More informationTowards a quantum treatment of leptogenesis
SEWM Swansea, July 10 13 2012 based on work in collaboration with Tibor Frossard, Andreas Hohenegger, Alexander Kartavtsev, Manfred Lindner [mainly 1112.6428] Physics beyond the Standard Model Collider
More informationStatus Report on Electroweak Baryogenesis
Outline Status Report on Electroweak Baryogenesis Thomas Konstandin KTH Stockholm hep-ph/0410135, hep-ph/0505103, hep-ph/0606298 Outline Outline 1 Introduction Electroweak Baryogenesis Approaches to Transport
More informationCosmological Family Asymmetry and CP violation
Cosmological Family Asymmetry and CP violation Satoru Kaneko (Ochanomizu Univ.) 2005. 9. 21 at Tohoku Univ. T. Endoh, S. K., S.K. Kang, T. Morozumi, M. Tanimoto, PRL ( 02) T. Endoh, T. Morozumi, Z. Xiong,
More informationDynamical CP violation in the Early Universe
Dynamical CP violation in the Early Universe Balaji Katlai (McGill University) In collaboration with T. Biswas, R.H. Brandenberger, David London Phys.Lett. B595, 22 (2004) DESY workshop, 2004. p.1/10 .
More informationLeptogenesis from a First-Order Lepton- Number Breaking Phase Transition
Leptogenesis from a First-Order Lepton- umber Breaking Phase Transition Andrew Long TeVPA 2017 at Ohio State University Aug 10, 2017 based on work with Andrea Tesi & Lian-Tao Wang (1703.04902 & JHEP) Bubbles!
More informationNonequilibrium dynamics and transport near the chiral phase transition of a quark-meson model
FAIRNESS 2013, 15-21 September 1 Nonequilibrium dynamics and transport near the chiral phase transition of a quark-meson model A Meistrenko 1, C Wesp 1, H van Hees 1,2 and C Greiner 1 1 Institut für Theoretische
More informationarxiv: v2 [hep-ph] 25 Aug 2009
Preprint typeset in JHEP style - PAPER VERSIO CER-PH-TH/2009-07 MPP-2009-85 PITHA 09/5 arxiv:0907.0205v2 hep-ph] 25 Aug 2009 Full Boltzmann equations for leptogenesis including scattering F. Hahn-Woernle,
More informationElectromagnetic Leptogenesis at TeV scale. Sudhanwa Patra
Electromagnetic Leptogenesis at TeV scale Sudhanwa Patra Physical Research Laboratory, INDIA Collaboration with Debjyoti Choudhury, Namit Mahajan, Utpal Sarkar 25th Feb, 2011 Sudhanwa Patra, NuHorizon-IV,
More informationFalsifying High-Scale Leptogenesis at the LHC
Falsifying High-Scale Leptogenesis at the LHC based on Frank F. Deppisch, JH, Martin Hirsch Phys. Rev. Lett. 112, 221601 (2014), arxiv: 1312.4447 [hep-ph] University College London 21/07/2104 SUSY 2014,
More informationBaryogenesis. David Morrissey. SLAC Summer Institute, July 26, 2011
Baryogenesis David Morrissey SLAC Summer Institute, July 26, 2011 Why is There More Matter than Antimatter? About 5% of the energy density of the Universe consists of ordinary (i.e. non-dark) matter. By
More informationThe Origin of Matter
The Origin of Matter ---- Leptogenesis ---- Tsutomu T. Yanagida (IPMU, Tokyo) Shoichi Sakata Centennial Symposium Energy Content of the Universe いいい From Wikipedia F FF Galaxy and Cluster of galaxies No
More informationElectroweak baryogenesis in the two Higgs doublet model
Michael Seniuch Bielefeld University 1 Electroweak baryogenesis in the two Higgs doublet model M. Seniuch, Bielefeld University COSMO 05 Bonn August 2005 Work is done in collaboration with Lars Fromme
More informationarxiv: v1 [hep-ph] 2 Jun 2015
TeV Scale Leptogenesis P. S. Bhupal Dev arxiv:1506.00837v1 [hep-ph] 2 Jun 2015 Abstract This is a mini-review on the mechanism of leptogenesis, with a special emphasis on low-scale leptogenesis models
More informationInterplay of flavour and CP symmetries
p. 1/79 Interplay of flavour and CP symmetries C. Hagedorn EC Universe, TUM, Munich, Germany ULBPhysTh Seminar, Université Libre de Bruxelles, 28.03.2014, Brussels, Belgium p. 2/79 Outline lepton mixing:
More informationLeptogenesis with Majorana neutrinos
Leptogenesis with Majorana neutrinos E.A. Paschos a a Institut für Physik, Universität Dortmund D-4422 Dortmund, Germany I review the origin of the lepton asymmetry which is converted to a baryon excess
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 informationSOME COMMENTS ON CP-VIOLATION AND LEPTOGENESIS
Marco Drewes TU München 23. 8. 2016, NuFact, Quy Nhon, Vietnam 1 / 7 The Standard Model and General Relativity together explain almost all phenomena observed in nature, but... gravity is not quantised
More informationLeptogenesis via Higgs Condensate Relaxation
The Motivation Quantum Fluctuations Higgs Relaxation Leptogenesis Summary Leptogenesis via Higgs Condensate Relaxation Louis Yang Department of Physics and Astronomy University of California, Los Angeles
More informationTesting leptogenesis at the LHC
Santa Fe Summer Neutrino Workshop Implications of Neutrino Flavor Oscillations Santa Fe, New Mexico, July 6-10, 2009 Testing leptogenesis at the LHC ArXiv:0904.2174 ; with Z. Chacko, S. Granor and R. Mohapatra
More informationElectroweak Baryogenesis in the LHC era
Electroweak Baryogenesis in the LHC era Sean Tulin (Caltech) In collaboration with: Michael Ramsey-Musolf Dan Chung Christopher Lee Vincenzo Cirigliano Bjorn Gabrecht Shin ichiro ichiro Ando Stefano Profumo
More informationThe Matter-Antimatter Asymmetry and New Interactions
The Matter-Antimatter Asymmetry and New Interactions The baryon (matter) asymmetry The Sakharov conditions Possible mechanisms A new very weak interaction Recent Reviews M. Trodden, Electroweak baryogenesis,
More informationNeutrino Masses SU(3) C U(1) EM, (1.2) φ(1, 2) +1/2. (1.3)
Neutrino Masses Contents I. The renormalizable Standard Model 1 II. The non-renormalizable Standard Model III. The See-Saw Mechanism 4 IV. Vacuum Oscillations 5 V. The MSW effect 7 VI. Experimental results
More informationNeutrinos and Cosmos. Hitoshi Murayama (Berkeley) Texas Conference at Stanford Dec 17, 2004
Neutrinos and Cosmos Hitoshi Murayama (Berkeley) Texas Conference at Stanford Dec 17, 2004 Outline A Little Historical Perspective Interpretation of Data & Seven Questions Matter Anti-Matter Asymmetry
More informationNeutrino theory of everything? dark matter, baryogenesis and neutrino masses
Neutrino theory of everything? dark matter, baryogenesis and neutrino masses 25 th International Workshop on Weak Interactions and Neutrinos (WIN2015) June 8-13, 2015, MPIK Heidelberg, Germany @Heidelberg
More informationNonrenormalizability of nonequilibrium quantum field theory in the classical approximation
Nonrenormalizability of nonequilibrium quantum field theory in the classical approximation Bin Wu IPhT, CEA/Saclay RPP 2015, Institut Henri Poincare Jan 16, 2015 T. Epelbaum, F. Gelis and B. Wu, Phys.
More informationBaryo- and leptogenesis. Purpose : explain the current excess of matter/antimatter. Is there an excess of matter?
Baryo- and leptogenesis Purpose : explain the current excess of matter/antimatter Is there an excess of matter? Baryons: excess directly observed; Antibaryons seen in cosmic rays are compatible with secondary
More informationTesting the low scale seesaw and leptogenesis
based on 1606.6690 and 1609.09069 with Marco Drewes, Björn Garbrecht and Juraj Klarić Bielefeld, 18. May 2017 Remaining puzzles of the universe BAU baryon asymmetry of the universe WMAP, Planck and Big
More informationKinetic approach to electroweak baryogenesis. Tomislav Prokopec
HD-THEP-0-07 Kinetic approach to electroweak baryogenesis Tomislav Prokopec Kimmo Kainulainen, Michael G. Schmidt and Steffen Weinstock Institut für Theoretische Physik, Universität Heidelberg Philosophenweg
More informationCreating Matter-Antimatter Asymmetry from Dark Matter Annihilations in Scotogenic Scenarios
Creating Matter-Antimatter Asymmetry from Dark Matter Annihilations in Scotogenic Scenarios Based on arxiv:1806.04689 with A Dasgupta, S K Kang (SeoulTech) Debasish Borah Indian Institute of Technology
More informationLeptogenesis via the Relaxation of Higgs and other Scalar Fields
Leptogenesis via the Relaxation of Higgs and other Scalar Fields Louis Yang Department of Physics and Astronomy University of California, Los Angeles PACIFIC 2016 September 13th, 2016 Collaborators: Alex
More informationThe first one second of the early universe and physics beyond the Standard Model
The first one second of the early universe and physics beyond the Standard Model Koichi Hamaguchi (University of Tokyo) @ Colloquium at Yonsei University, November 9th, 2016. Credit: X-ray: NASA/CXC/CfA/M.Markevitch
More informationElectroweak Baryogenesis A Status Report
Electroweak Baryogenesis A Status Report Thomas Konstandin Odense, August 19, 2013 review: arxiv:1302.6713 Outline Introduction SUSY Composite Higgs Standard Cosmology time temperature Standard Cosmology
More informationThermal Quantum Field Theory in Real and Imaginary Time. Daniele Teresi
Thermal Quantum Field Theory in Real and Imaginary Time daniele.teresi@hep.manchester.ac.uk University of Manchester 42nd BUSSTEPP - Durham University WHAT IS THERMAL QFT? ORDINARY VACUUM QFT few in and
More informationQUANTUM KINETIC THEORY WITH NONLOCAL COHERENCE BY MATTI HERRANEN
DEPARTMENT OF PHYSICS UNIVERSITY OF JYVÄSKYLÄ RESEARCH REPORT No. 3/2009 QUANTUM KINETIC THEORY WITH NONLOCAL COHERENCE BY MATTI HERRANEN Academic Dissertation for the Degree of Doctor of Philosophy To
More informationFalsifying highscale Baryogenesis
ILP - LPTHE - UPMC - CNRS Paris in collaboration with F. Deppisch, L. Graf, W. Huang, M. Hirsch, H. Päs F. Deppisch, JH, M. Hirsch, PRL 112 (2014) 221601 ACFI Workshop F. Deppisch, JH, W. Huang, M. Hirsch,
More informationLepton Number Violation and the Baryon Asymmetry of the Universe
Lepton Number Violation and the Baryon Asymmetry of the Universe ILP / LPTHE Paris ACFI Workshop, 29.03.2018 F. Deppisch, L. Graf, JH, W. Huang, arxiv:1711.10432 F. Deppisch, JH, W. Huang, M. Hirsch, H.
More informationNeutrino masses. Universe
Università di Padova,, 8 May, 2008 Neutrino masses and the matter-antimatter antimatter asymmetry of the Universe (new results in collaboration with Steve Blanchet to appear soon) Pasquale Di Bari (INFN,
More informationQuantum transport and electroweak baryogenesis
Quantum transport and electroweak baryogenesis Thomas Konstandin Mainz, August 7, 2014 review: arxiv:1302.6713 Outline Introduction MSSM Composite Higgs Baryogenesis [Sakharov '69] Baryogenesis aims at
More informationWhat We Know, and What We Would Like To Find Out. Boris Kayser Minnesota October 23,
What We Know, and What We Would Like To Find Out Boris Kayser Minnesota October 23, 2008 1 In the last decade, observations of neutrino oscillation have established that Neutrinos have nonzero masses and
More informationPhase transitions in cosmology
Phase transitions in cosmology Thomas Konstandin FujiYoshida, August 31, 2017 Electroweak phase transition gravitational waves baryogenesis Outline Introduction MSSM Composite Higgs Baryogenesis [Sakharov
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 informationNatural Nightmares for the LHC
Dirac Neutrinos and a vanishing Higgs at the LHC Athanasios Dedes with T. Underwood and D. Cerdeño, JHEP 09(2006)067, hep-ph/0607157 and in progress with F. Krauss, T. Figy and T. Underwood. Clarification
More informationNeutrino masses, muon g-2, dark matter, lithium probelm, and leptogenesis at TeV-scale SI2009 AT FUJI-YOSHIDA
Neutrino masses, muon g-2, dark matter, lithium probelm, and leptogenesis at TeV-scale SI2009 AT FUJI-YOSHIDA Chian-Shu Chen National Cheng Kung U./Academia Sinica with C-H Chou 08/20/2009 arxiv:0905.3477
More informationLepton Number Violation
and the Baryon Asymmetry of the Universe - - tu dortmund MPI Seminar Max-Planck-Institut für Kernphysik Heidelberg December 14, 2015 Outline The Baryon Asymmetry of the Universe (LNV) Double Beta Decay
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 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 informationPOST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY
POST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY LOUIS YANG ( 楊智軒 ) UNIVERSITY OF CALIFORNIA, LOS ANGELES (UCLA) DEC 30, 2016 4TH INTERNATIONAL WORKSHOP ON DARK MATTER,
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 informationELECTRIC DIPOLE MOMENT OF THE ELECTRON AND ITS COSMOLOGICAL IMPLICATIONS
ELECTRIC DIPOLE MOMENT OF THE ELECTRON AND ITS COSMOLOGICAL IMPLICATIONS H S NATARAJ Under the Supervision of Prof. B P DAS Non-Accelerator Particle Physics Group Indian Institute of Astrophysics Bangalore
More informationSelf-consistent Conserving Approximations and Renormalization in Quantum Field Theory at Finite Temperature
Self-consistent Conserving Approximations and Renormalization in Quantum Field Theory at Finite Temperature Hendrik van Hees in collaboration with Jörn Knoll Contents Schwinger-Keldysh real-time formalism
More information12 Best Reasons to Like CP Violation
12 Best Reasons to Like CP Violation SSI 2012 The Electroweak Scale: Unraveling the Mysteries at the LHC SLAC, California 27 July 2012 Yossi Nir (Weizmann Institute of Science) SSI40 1/35 CP Violation
More informationTime evolution of particle number asymmetry in an expanding universe
Time evolution of particle number asymmetry in an expanding universe Apriadi Salim Adam In collaboration with: Takuya Morozumi, Keiko Nagao, Hiroyuki Takata Graduate School of Science, Hiroshima University
More informationPuzzles of Neutrinos and Anti-Matter: Hidden Symmetries and Symmetry Breaking. Hong-Jian He
Puzzles of Neutrinos and Anti-Matter: Hidden Symmetries and Symmetry Breaking Tsinghua University 2009-1-13 Collaborators: Shao-Feng Ge & Fu-Rong Yin Based on arxiv:1001.0940 (and works in preparation)
More informationNeutrino Mass Seesaw, Baryogenesis and LHC
Neutrino Mass Seesaw, Baryogenesis and LHC R. N. Mohapatra University of Maryland Interplay of Collider and Flavor Physics workshop, CERN Blanchet,Chacko, R. N. M., 2008 arxiv:0812:3837 Why? Seesaw Paradigm
More informationEquilibration in ϕ 4 theory in 3+1 dimensions
Equilibration in ϕ 4 theory in 3+1 dimensions Alejandro Arrizabalaga Work in collaboration with Anders Tranberg (Sussex) and Jan Smit (Amsterdam) Physical Review D 72 020514 (2005) NIKHEF (Amsterdam) Summer
More informationLight Stop Bound State Production at the LHC. Yeo Woong Yoon (KIAS) In collaboration with P. Ko, Chul Kim at Yonsei U.
Light Stop Bound State Production at the LHC Yeo Woong Yoon (KIAS) In collaboration with P. Ko, Chul Kim 0. 6. 8 at Yonsei U. Outline About stop Motivation for light stop Phenomenology Formalism Summary
More informationElectroweak baryogenesis in light of the Higgs discovery
Electroweak baryogenesis in light of the Higgs discovery Thomas Konstandin Grenoble, March 25, 2013 review: arxiv:1302.6713 Outline Introduction SUSY Composite Higgs Baryogenesis [Sakharov '69] Baryogenesis
More informationBaryogenesis and Particle Antiparticle Oscillations
Baryogenesis and Particle Antiparticle Oscillations Seyda Ipek UC Irvine SI, John March-Russell, arxiv:1604.00009 Sneak peek There is more matter than antimatter - baryogenesis SM cannot explain this There
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 informationgeneration Outline Outline Motivation Electroweak constraints Selected flavor constraints in B and D sector Conclusion Nejc Košnik
th Discovery Discovery of of the the 4 4th generation generation Outline Outline Motivation Electroweak constraints Selected flavor constraints in B and D sector Conclusion 1 Introduction Introduction
More informationElectroweak phase transition with two Higgs doublets near the alignment limit
Electroweak phase transition with two Higgs doublets near the alignment limit Jérémy Bernon The Hong Kong University of Science and Technology Based on 1712.08430 In collaboration with Ligong Bian (Chongqing
More informationHidden Sector Baryogenesis. Jason Kumar (Texas A&M University) w/ Bhaskar Dutta (hep-th/ ) and w/ B.D and Louis Leblond (hepth/ )
Hidden Sector Baryogenesis Jason Kumar (Texas A&M University) w/ Bhaskar Dutta (hep-th/0608188) and w/ B.D and Louis Leblond (hepth/0703278) Basic Issue low-energy interactions seem to preserve baryon
More informationZhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016
Zhong-Zhi Xianyu (CMSA Harvard) Tsinghua June 30, 2016 We are directly observing the history of the universe as we look deeply into the sky. JUN 30, 2016 ZZXianyu (CMSA) 2 At ~10 4 yrs the universe becomes
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 informationLeptogenesis: Improving predictions for experimental searches
: Improving predictions for experimental searches Physik Department T70, Technische Universität München, James Franck Straße 1, D-85748 E-mail: marco.drewes@tum.de Björn Garbrecht Physik Department T70,
More informationNon-local 1/m b corrections to B X s γ
Non-local 1/m b corrections to B X s γ Michael Benzke TU München September 16, 2010 In collaboration with S. J. Lee, M. Neubert, G. Paz Michael Benzke (JGU) Non-local 1/m b corrections to B X s γ TU München
More informationarxiv:hep-ph/ v6 3 Apr 2001
CP Violation in Seesaw Model T. Endoh, T. Morozumi, T. Onogi and A. Purwanto arxiv:hep-ph/00345v6 3 Apr 00 Department of Physics, Hiroshima University -3- Kagamiyama, Higashi Hiroshima - 739-856, Japan
More informationSymmetric WIMP Dark Matter and Baryogenesis
Symmetric WIMP Dark Matter and Baryogenesis based on NB, François-Xavier Josse-Michaux and Lorenzo Ubaldi To appear soon... Nicolás BERNAL Bethe Center for Theoretical Physics and Physikalisches Institut
More informationElectroweak Baryogenesis in Non-Standard Cosmology
Electroweak Baryogenesis in Non-Standard Cosmology Universität Bielefeld... KOSMOLOGIETAG 12... Related to works in colloboration with M. Carena, A. Delgado, A. De Simone, M. Quirós, A. Riotto, N. Sahu,
More informationA Brief History of Modern Physics
A Brief History of Modern Physics Modern Physics rests on two pillars: 1. Theory of Relativity (Einstein) Special Relativity 1905 General Relativity 1915 nature of space and time (phenomena at high speed)
More informationarxiv:hep-ph/ v1 20 Mar 2002
Resurrection of Grand Unified Theory Baryogenesis M. Fukugita 1 and T. Yanagida 2 1 Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 2778582, Japan arxiv:hep-ph/0203194v1 20 Mar 2002 Abstract
More informationLeptogenesis and the Flavour Structure of the Seesaw
Leptogenesis and the Flavour Structure of the Seesaw based on: hep-ph/0609038 (JCAP 0611 (2006) 011) with S.F. King, A. Riotto hep-ph/0611232 (JCAP 0702 (2007) 024) with A.M. Teixeira arxiv:0704.1591 (Phys.
More informationarxiv:hep-ph/ v1 26 Jul 2006
Neutrino mass and baryogenesis arxiv:hep-ph/0607287v1 26 Jul 2006 D. Falcone Dipartimento di Scienze Fisiche, Università di Napoli, Via Cintia, Napoli, Italy A brief overview of the phenomenology related
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 informationWho is afraid of quadratic divergences? (Hierarchy problem) & Why is the Higgs mass 125 GeV? (Stability of Higgs potential)
Who is afraid of quadratic divergences? (Hierarchy problem) & Why is the Higgs mass 125 GeV? (Stability of Higgs potential) Satoshi Iso (KEK, Sokendai) Based on collaborations with H.Aoki (Saga) arxiv:1201.0857
More informationElectroweak baryogenesis in the MSSM and nmssm
Electroweak baryogenesis in the MSSM and nmssm Thomas Konstandin, IFAE Barcelona in collaboration with S. Huber, T. Prokopec, M.G. Schmidt and M. Seco Outline 1 Introduction The Basic Picture 2 Semiclassical
More informationCosmology at Colliders: Possible LHC searches for RPV baryogenesis
Cosmology at Colliders: Possible LHC searches for RPV baryogenesis Haipeng An Perimeter Ins;tute In collaboration with Yue Zhang arxiv:1310.2608 Mo;va;ons We are made of baryons and we have been living
More informationGrand Unification. Strong, weak, electromagnetic unified at Q M X M Z Simple group SU(3) SU(2) U(1) Gravity not included
Pati-Salam, 73; Georgi-Glashow, 74 Grand Unification Strong, weak, electromagnetic unified at Q M X M Z Simple group G M X SU(3) SU() U(1) Gravity not included (perhaps not ambitious enough) α(q ) α 3
More informationElectroweak phase transition in the early universe and Baryogenesis
Electroweak phase transition in the early universe and Baryogenesis Arka Banerjee December 14, 2011 Abstract In the Standard Model, it is generally accepted that elementary particles get their masses via
More informationHiggs Physics and Cosmology
Higgs Physics and Cosmology Koichi Funakubo Department of Physics, Saga University 1 This year will be the year of Higgs particle. The discovery of Higgs-like boson will be reported with higher statistics
More informationThe Origin of Matter. Koichi Funakubo Dept. Physics Saga University. NASA Hubble Space Telescope NGC 4911
The Origin of Matter Koichi Funakubo Dept. Physics Saga University NASA Hubble Space Telescope NGC 4911 fundamental theory of elementary particles Local Quantum Field Theory causality relativistic quantum
More informationTheory of CP Violation
Theory of CP Violation IPPP, Durham CP as Natural Symmetry of Gauge Theories P and C alone are not natural symmetries: consider chiral gauge theory: L = 1 4 F µνf µν + ψ L i σdψ L (+ψ R iσ ψ R) p.1 CP
More informationSuccessful Leptogenesis in the Left-Right Symmetric Seesaw Mechanism
Successful Leptogenesis in the Left-Right Symmetric Seesaw Mechanism Pierre Hosteins Patras University 13th November 2007 Brussels P.H., S. Lavignac and C. Savoy, Nucl. Phys. B755, arxiv:hep-ph/0606078
More informationCP Violation, Baryon violation, RPV in SUSY, Mesino Oscillations, and Baryogenesis
CP Violation, Baryon violation, RPV in SUSY, Mesino Oscillations, and Baryogenesis David McKeen and AEN, arxiv:1512.05359 Akshay Ghalsasi, David McKeen, AEN., arxiv:1508.05392 (Thursday: Kyle Aitken, David
More informationAstroparticle Physics and the LC
Astroparticle Physics and the LC Manuel Drees Bonn University Astroparticle Physics p. 1/32 Contents 1) Introduction: A brief history of the universe Astroparticle Physics p. 2/32 Contents 1) Introduction:
More informationPOST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY
POST-INFLATIONARY HIGGS RELAXATION AND THE ORIGIN OF MATTER- ANTIMATTER ASYMMETRY LOUIS YANG ( 楊智軒 ) UNIVERSITY OF CALIFORNIA, LOS ANGELES (UCLA) DEC 27, 2016 NATIONAL TSING HUA UNIVERSITY OUTLINE Big
More information