Duality in left-right symmetric seesaw
|
|
- Mervyn Webster
- 5 years ago
- Views:
Transcription
1 Duality in left-right symmetric seesaw Evgeny Akhmedov KTH, Stockholm & Kurchatov Institute, Moscow In collaboration with Michele Frigerio Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 1
2 Why are neutrinos so light? A simple and elegant explanation The seesaw mechanism (Minkowski, 1977; Gell-Mann, Ramond & Slansky, 1979; Yanagida, 1979; Glashow, 1979; Mohapatra & Senjanović, 1980) In addition: Seesaw has a built-in mechanism for generating the baryon asymmetry of the Universe Baryogenesis via Leptogenesis (Fukugita & Yanagida, 1986; Luty, 1992; Covi et al., 1996; Buchmüller & Plümacher, 1996;...) The simplest version: Add 3 RH ν s N Ri yo the minimal SM Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 2
3 Heavy N Ri s make ν Li s light : L Y +m = Y ν ll N R H M RN R N R + h.c., Neutrino mass matrix in the (ν L, (N R ) c ) basis: M ν = 0 m D m T D M R N Ri are EW singlets M R M GUT (M I ) m D v. Block diagonalization: M N M R, m νl m D M 1 R mt D m ν (174 GeV)2 M R For m ν 0.05 ev M R GeV M GUT GeV! Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 3
4 Type II seesaw Type I seesaw: Neutrino mass generated through exchage of a heavy RH ν s N R ; in type II through exchage of a heavy SU(2) L - triplet scalars L : In the SM, RH neutrinos N R are singlets of the gauge group aliens. They are more natural in Left-Right symmetric extensions of the SM: SU(2) L SU(2) R U(1) B L, SU(2) L SU(2) R SU(4) PS, SO(10),... LR symmetric models explain in a nice way maximal P- and C-violation in low-e weak interactions as a spontaneous symmetry breaking phenomenon likely to be present in the final theory Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 4
5 In LR - symmetric models: In general, both type I and type II seesaw contributions to m ν are present : M ν = Block diagonalization of M ν : m L m T D m D M R m ν m L m D M 1 R mt D m D comes from Yukawa interactions with the bi-doublet Higgs Φ: Y 1 ll Φ l R + Y 2 ll Φ l R, Φ τ 2 Φ τ 2 m D = yv m L and M R from Yukawa couplings with triplet Higgses L and R m ν f L v L v 2 y (f R v R ) 1 y T In general: m ν, f L and f R complex symmetric, y complex matrix Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 5
6 Parity symmetry Discrete LR symmetry (P) in LR-symm. models two possible implementations: (1) l Li l Ri, L R, Φ Φ Yields f L = f R, y = y, (2) l Li l c Li (l Ri ) c, L R, Φ Φ T Yields f L = f R f, y = y T. Both implementations possible. Implem. (2) is more natural in SO(10) GUTs (is an automatic gauge symmetry) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 6
7 Adhere to the second implementation m ν = fv L v 2 y (v R f) 1 y For realization (1) of parity: type I term contains (f ) 1 instead of f 1. N R, R, L are all at very high scale ( GeV) no direct way of probing this sector of the theory. Neutrinos may provide a low-energy window into new physics at very high energy scales! Take m ν from experiment Bottom-up approach: Take y from data + theoretical assumptions (quark-lepton symm., GUTs) Solve the seesaw relation for f E.A. and M. Frigerio, PRL 96 (2006) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 7
8 What would we like to know? Try to learn as much as possible about the heavy neutrino sector What are the masses of heavy RH neutrinos? What are the mixing and CP violation in the heavy RH neutrino sector? Can all this give us a hint of the underlying theory? Is the solution that we found unique? Is type I or type II contribution in the light neutrino mass dominant or are they equally important? Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 8
9 Inverting the seesaw formula Pure type I (c 0 v 2 /v R ): m ν = c 0 ( y f 1 y T) f = c 0 ( y T m 1 ν y ) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 9
10 Inverting the seesaw formula Pure type I (c 0 v 2 /v R ): Pure type II: m ν = c 0 ( y f 1 y T) f = c 0 ( y T m 1 ν y ) m ν = f v L f = m ν /v L Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 9
11 Inverting the seesaw formula Pure type I (c 0 v 2 /v R ): Pure type II: m ν = c 0 ( y f 1 y T) f = c 0 ( y T m 1 ν y ) m ν = f v L f = m ν /v L General type I + II seesaw: m ν = fv L v2 v R ( y f 1 y ) a nonlinear matrix equation for f. Yet can be readily solved analytically! Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 9
12 Inverting the seesaw formula Pure type I (c 0 v 2 /v R ): Pure type II: m ν = c 0 ( y f 1 y T) f = c 0 ( y T m 1 ν y ) m ν = f v L f = m ν /v L General type I + II seesaw: m ν = fv L v2 v R ( y f 1 y ) a nonlinear matrix equation for f. Yet can be readily solved analytically! Important point: A duality property of LR-symmetric seesaw If f is a solution, so is ˆf (m ν /v L f) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 9
13 Inverting the seesaw formula Pure type I (c 0 v 2 /v R ): Pure type II: m ν = c 0 ( y f 1 y T) f = c 0 ( y T m 1 ν y ) m ν = f v L f = m ν /v L General type I + II seesaw: m ν = fv L v2 v R ( y f 1 y ) a nonlinear matrix equation for f. Yet can be readily solved analytically! Important point: A duality property of LR-symmetric seesaw If f is a solution, so is ˆf (m ν /v L f) There is always an even number of solutions! (#sol. = 2 n ) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 9
14 LR symmetry important for duality! It was important that f L = f R and y T = y. For the other realization of parity symmetry (f L = f R and y = y ) exactly the same duality holds! f 1 = 1 F Two-generation case f 22 f 12 f 12 f 11, y = y e2 y e1 y µ1 y µ2, F detf, y µ1 = y e2. Define: x v L v R /v 2 and m m ν /v L xf(f 11 m ee ) = f 22 ye1 2 2f 12 y e1 y e2 + f 11 ye2 2, xf(f 22 m µµ ) = f 22 ye2 2 2f 12 y e2 y µ2 + f 11 yµ2 2, xf(f 12 m eµ ) = f 22 y e1 y e2 f 12 (y e1 y µ2 + ye2) 2 + f 11 y e2 y µ2, Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 10
15 A system of coupled 3rd order equations Admits a simple exact analytic solution! Go to the basis where y is diagonal: y = diag(y 1, y 2 ) (no loss of generality) xf(f 11 m ee ) = f 22 y 2 1 xf(f 22 m µµ ) = f 11 y 2 2 xf(f 12 m eµ ) = f 12 y 1 y 2 Rescaling: f ij = λf ij, m ij = λm ij, y ij = λy ij, λ - arbitrary; fix it by requiring F detf = 1. The system of eqs. for f ij becomes linear Express f ij back through unprimed m ij, y 1,2 and subst. into F 4th order characteristic equation for λ = 1 Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 11
16 The solution: f = xλ (xλ) 2 y 2 1 y2 2 xλm ee + y1m 2 µµ m eµ (xλ y 1 y 2 )... xλm µµ + y2m 2 ee λ has to be found from [ (xλ) 2 y1y ] 2 [ x detm(xλ y1 y 2 ) 2 xλ +(m ee y 2 + m µµ y 1 ) 2 (xλ) 2] = 0 Has 4 complex solutions 4 solutions for f which form 2 dual pairs Determinant of the seesaw relation x ˆf = yf 1 y x 2 F ˆF = y 2 1y 2 2 F = 1 F = λ; therefore x 2 λˆλ = y 2 1y 2 2 Allows to express the four solutions for λ in a simple closed form Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 12
17 Which seesaw type dominates? If m αβ m γδ 4 y i y j /x, one of the solutions λ i satisfies xλ 1 y i y j f 1 m (type II seesaw) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 13
18 Which seesaw type dominates? If m αβ m γδ 4 y i y j /x, one of the solutions λ i satisfies xλ 1 y i y j f 1 m (type II seesaw) Then for the dual solution λ 2 : xλ 2 y i y j f 2 = ˆf 1 corresponds to type I seesaw The remaining 2 solutions are of mixed type. Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 13
19 Which seesaw type dominates? If m αβ m γδ 4 y i y j /x, one of the solutions λ i satisfies xλ 1 y i y j f 1 m (type II seesaw) Then for the dual solution λ 2 : xλ 2 y i y j f 2 = ˆf 1 corresponds to type I seesaw The remaining 2 solutions are of mixed type. If m αβ m γδ 4 y i y j /x, all 4 solutions are of mixed type. Similar situation in 3-generation case Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 13
20 Which seesaw type dominates? If m αβ m γδ 4 y i y j /x, one of the solutions λ i satisfies xλ 1 y i y j f 1 m (type II seesaw) Then for the dual solution λ 2 : xλ 2 y i y j f 2 = ˆf 1 corresponds to type I seesaw The remaining 2 solutions are of mixed type. If m αβ m γδ 4 y i y j /x, all 4 solutions are of mixed type. Similar situation in 3-generation case In general, if there is a solution with seesaw type I dominance, there is always also a solution with type II sessaw dominance and vice versa. Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 13
21 Which seesaw type dominates? If m αβ m γδ 4 y i y j /x, one of the solutions λ i satisfies xλ 1 y i y j f 1 m (type II seesaw) Then for the dual solution λ 2 : xλ 2 y i y j f 2 = ˆf 1 corresponds to type I seesaw The remaining 2 solutions are of mixed type. If m αβ m γδ 4 y i y j /x, all 4 solutions are of mixed type. Similar situation in 3-generation case In general, if there is a solution with seesaw type I dominance, there is always also a solution with type II sessaw dominance and vice versa. Using low-energy data only, it is impossible to say which seesaw type dominataes (if any) additional criteria necessary (leptogenesis?) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 13
22 Three lepton generations A system of six coupled 4th order equations can be readily solved analytically by making use of the same trick as in 2-g case plus duality. Characteristic equation for the rescaling factor λ is of 8th order 8 solutions λ i 8 solutions f i (i = 1,...,8). Form 4 pairs of mutually dual solutions For given y (i.e. m D ), all 8 solutions result in exactly the same mass matrix of light neutrinos m ν! Analysis of solutions under way Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 14
23 Conclusions In LR - symmetric models (minimal LR, Pati-Salam, SO(10). E 6,...) one naturally has type I + II seesaw mechanism of neutrino mass generation Discrete LR symmetry (parity) leads to a relation between type I and type II contributions to m ν, which results in a duality property of the seesaw formula: f m ν /v L f For given y, there are 2 n (8 for three lepton generations) matrices f which result in exactly the same mass matrix of light neutrinos m ν A simple analytic method developed for solving the seesaw nonlinear matrix equation. Allows bottom-up reconstraction of the Yukawa coupling matrix f of heavy RH neutrinos The results may be used for neutrino mass model building and studies of baryogenesis via leptogenesis. Allow to analytically explore the interplay of type I and II contributions to m ν Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 15
24 Backup slides Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 16
25 RGE issues The discrete LR (parity) symmetry of the underlying theory must be broken at some scale v LR renormalization group evolution below this scale may result in a violation of conditions f L = f R f, y = y T at lower energies. Corrections to matrix elements of y and f depend logarithmically on ratios of masses of RH neutrinos and Higgs triplets; are suppressed by loop factors and possibly by small couplings. Numerically checked: If LR-violating corrections to the matr. elements are of the order of percent, reconstruction of the matrix f remains accurate at a percent level. The stability may be lost if small matrix elements receive corrections proportional to the large elements a dedicated study necessary Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 17
26 Mass matrix of light neutrinos m ν Symmetric mass matrix diagonalized as m ν = U T m diag U, m diag = diag(m 1, m 2, m 3 ) The masses m i known up to the overall scale parameterized by m 1 : m 2 = m m2 21, m 3 = m m2 31 Leptonic mixing matrix U: U = c 23 s 23 0 s 23 c 23 c 13 0 s 13 e iδ s 13 e iδ 0 c 13 c 12 s 12 0 s 12 c e iα e iβ c ij cos θ ij, s ij sinθ ij Experiment: θ 12 34, θ 23 45, θ 13 < 10. CP violating phases can be varied between 0 and 2π. Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 18
27 The solutions in 2-generation case xλ i = 1 4 [xdetm + r ± ± 2(detm) 2 x 2 + 4kx + 2xr ± detm], where r ± = ± (detm) 2 x 2 + 4kx + 16y 2 1 y2 2, k = m 2 eey m 2 eµy 1 y 2 + m 2 µµy 2 1. When λ 1 satisfies xλ 1 y i y j f 1 m (type II seesaw case) The dual solution xλ 2 = xˆλ 1 = y1y 2 2/(xλ 2 1 ) has modulus y i y j f 2 = ˆf 1 takes type I seesaw form Condition xλ 1 y i y j can only be satisfied when m αβ m γδ 4 y i y j /x. This ensures the existence of solutions with one seesaw type dominance. But: in general not all 4 solutions correspond to one seesaw type dominance in this limit: if detm 4 y i y j /x, the remaining 2 dual solutions f 3 and f 4 are of mixed type. When m αβ m γδ 4 y i y j /x, all 4 sols. are of mixed type. Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 19
28 Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 20
29 Three lepton generations Once again go to the basis where y = diag(y 1, y 2, y 3 ). f 1 = 1 f 22 f 33 f F System of 6 coupled 4th order equations: xf (m 11 f 11 ) = y 2 1 (f 22 f 33 f 2 23)..... Simple rescaling would not do! Use similar equations for duals: x ˆF (m 11 ˆf 11 ) x ˆF f 11 = y 2 1 ( ˆf 22 ˆf33 ˆf 2 23) and ( ˆf 22 ˆf33 ˆf 2 23) = (m 22 f 22 )(m 33 f 33 ) (m 23 f 23 ) 2 Allows to express quadratic in f terms through linear and f-indep. terms and ˆF Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 21
30 Resulting system: x(f+ ˆF) f 11 = y1 2 [(m 22 m 33 m 2 23) (m 22 f 33 + m 33 f 22 2m 23 f 23 )] + xf m Now one can rescale: f ij = λ 1/3 f ij, m ij = λ 1/3 m ij, y ij = λ 1/3 y ij, Fix λ by requiring F detf = 1 Determinant condition: x 3 F ˆF = y 2 1 y 2 2 y 2 3 x 3 ˆF = (y 1 y 2 y 3) 2 System of 6 linear eqs. for f ij easily solved. Substitution into F = 1 (F = λ) 8th order characteristic eq. for λ. Yields 4 pairs of dual solutions for the matrix f. Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 22
31 3 generation case more details Equations for the matrix elements of f and its dual ˆf: xf(f ij m ij ) = y i y j F ij, (1) x ˆF( ˆf ij m ij ) = x ˆFf ij = y i y j ˆFij, (2) Here: F detf, ˆF det ˆf and F ij 1 2 ǫ iklǫ jmn f km f ln, ˆF ij 1 2 ǫ iklǫ jmn ˆfkm ˆfln = M ij T ij + F ij, M ij 1 2 ǫ iklǫ jmn m km m ln, T ij ǫ ikl ǫ jmn f km m ln. A system of 6 coupled quartic equations for f ij. RH sides are quadratic rather than linear in f ij a simple rescaling would not linearize the system. But: using the dual system of eqs. gives for these RH sides y i y j F ij = x ˆFf ij + y i y j (T ij M ij ) Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 23
32 Linearization: rescaling by a factor λ 1/3 Determinant condition: x 3 F ˆF = y 2 1 y 2 2 y 2 3. Fix λ by requiring F (λ) = 1; ˆF = (y 1y 2y 3) 2 /x 3. The linearized system: [x 3 (y 1y 2y 3) 2 ]f ij x 3 m ij = x 2 y iy j(t ij M ij). - Simplified case: y 1 0 (physically well motivated). The result: f 11 = m ee, f 12 = m eµ, f 13 = m eτ, ( f 23 = m µτ + y 2y 3 m eµ m ) eτ /d 2, xλ [ ( )] f 22 = m µµ + y2 2 M 22 y2 3m ee m 2 eµ xλ xλ [ ( f 33 = m ττ + y2 3 M 33 y2 2m ee m 2 eτ xλ xλ /d 1, )] /d 1, Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 24
33 Here: Characteristic equation for λ: d 1 = 1 y2 2y3m 2 2 ee (xλ) 2, d 2 = 1 + y 2y 3 m ee xλ. λ 4 { [(xλ) 2 m 2 eey 2 2y 2 3] 2 x [ detm(xλ m ee y 2 y 3 ) 2 xλ +(M 22 y 2 + M 33 y 3 ) 2 (xλ) 2]} = 0. If a solution λ of general charact. eq. 0 in the limit y 1 0, then ˆλ = y1y 2 2y 2 3/(x 2 3 λ) 0 determinant of ˆf vanishes. The dual of any solution that is finite for y 1 0 becomes singular and must be discarded. For y 1 0 there are only 4 (rather than 8) solutions with no duals. The corresp. values of λ are zeros of the factor in curly brackets (which is quartic in λ). Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 25
34 A strong connection with the pure 2-g case A different duality among the 4 remaining solutions: If λ satisfies the charact. equation, so does λ y 2 2y 2 3m 2 ee/(x 2 λ), and it corresponds to where f m f, m αβ = m αβ + m eα m eβ /m ee. There are two pairs of such solutions. Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 26
35 Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 27
36 Why is m ν = 0 in the Standard Model? No RH neutrinos N Ri Dirac mass terms cannot be introduced Operators of the kind l lhh, which could could produce Majorana neutrino mass after H H, are dimension 5 and so cannot be present at the Lagrangian level in a renormalizable theory These operators cannot be induced in higher orders either (even nonperturbatively) because they would break not only lepton number L but also B L, which is exactly conserved in the SM In the Standard Model: B and L are accidental symmetries at the Lagrangian level. Get broken at 1-loop level due the axial (triangle) anomaly. But: their difference B L is still conserved and is an exact symmetry of the model Evgeny Akhmedov SNOW 2006 Stockholm May 4, 2006 p. 28
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 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 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 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 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 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 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 informationPuzzles of Neutrino Mixing and Anti-Matter: Hidden Symmetries and Symmetry Breaking. Shao-Feng Ge
Puzzles of Neutrino Mixing and Anti-Matter: Hidden Symmetries and Symmetry Breaking Shao-Feng Ge (gesf02@mails.thu.edu.cn) Center for High Energy Physics, Tsinghua Univeristy 200-4-8 Collaborators: Hong-Jian
More informationA Novel and Simple Discrete Symmetry for Non-zero θ 13
A Novel and Simple Discrete Symmetry for Non-zero θ 13 Yang-Hwan, Ahn (KIAS) Collaboration with Seungwon Baek and Paolo Gondolo NRF workshop Yonsei Univ., Jun 7-8, 2012 Contents Introduction We propose
More informationTheoretical Models of neutrino parameters. G.G.Ross, Paris, September 2008
Theoretical Models of neutrino parameters. G.G.Ross, Paris, September 2008 Theoretical Models of neutrino parameters. G.G.Ross, Paris, September 2008 Number of light neutrinos 3? Masses + Mixing Angles
More informationF. Börkeroth, F. J. de Anda, I. de Medeiros Varzielas, S. F. King. arxiv:
F. Börkeroth, F. J. de Anda, I. de Medeiros Varzielas, S. F. King S FLASY 2015 arxiv:1503.03306 Standard Model Gauge theory SU(3)C X SU(2)L X U(1)Y Standard Model Gauge theory SU(3)C X SU(2)L X U(1)Y SM:
More informationThe Standard Model and beyond
The Standard Model and beyond In this chapter we overview the structure of the Standard Model (SM) of particle physics, its shortcomings, and different ideas for physics beyond the Standard Model (BSM)
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 informationJIGSAW 07. Neutrino Mixings and Leptonic CP Violation from CKM Matrix and Majorana Phases. Sanjib Kumar Agarwalla
JIGSAW 07 Neutrino Mixings and Leptonic CP Violation from CKM Matrix and Majorana Phases Sanjib Kumar Agarwalla Harish-Chandra Research Institute, Allahabad, India work done in collaboration with M. K.
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 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 informationSM predicts massless neutrinos
MASSIVE NEUTRINOS SM predicts massless neutrinos What is the motivation for considering neutrino masses? Is the question of the existence of neutrino masses an isolated one, or is connected to other outstanding
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 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 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 informationSUSY models of neutrino masses and mixings: the left-right connection
SUSY models of neutrino masses and mixings: the left-right connection GK Workshop Bad Liebenzell Wolfgang Gregor Hollik October 10, 2012 INSTITUT FÜR THEORETISCHE TEILCHENPHYSIK KIT CAMPUS SÜD KIT University
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 informationAutomatic CP Invariance and Flavor Symmetry
PRL-TH-95/21 Automatic CP Invariance and Flavor Symmetry arxiv:hep-ph/9602228v1 6 Feb 1996 Gautam Dutta and Anjan S. Joshipura Theory Group, Physical Research Laboratory Navrangpura, Ahmedabad 380 009,
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 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 informationLepton Flavor Violation
Lepton Flavor Violation I. The (Extended) Standard Model Flavor Puzzle SSI 2010 : Neutrinos Nature s mysterious messengers SLAC, 9 August 2010 Yossi Nir (Weizmann Institute of Science) LFV 1/39 Lepton
More informationarxiv:hep-ph/ v1 5 Oct 2005
Preprint typeset in JHEP style - HYPER VERSION RITS-PP-003 arxiv:hep-ph/0510054v1 5 Oct 2005 Constraint on the heavy sterile neutrino mixing angles in the SO10) model with double see-saw mechanism Takeshi
More informationScaling in the Neutrino Mass Matrix and the See-Saw Mechanism. Werner Rodejohann (MPIK, Heidelberg) Erice, 20/09/09
Scaling in the Neutrino Mass Matrix and the See-Saw Mechanism Werner Rodejohann (MPIK, Heidelberg) Erice, 20/09/09 1 A. S. Joshipura, W.R., Phys. Lett. B 678, 276 (2009) [arxiv:0905.2126 [hep-ph]] A. Blum,
More informationCOLLIDER STUDIES OF HIGGS TRIPLET MODEL
Miami 2010 December 16, 2010 COLLIDER STUDIES OF HIGGS TRIPLET MODEL Cheng-Wei Chiang National Central Univ. and Academia Sinica (on leave at Univ. of Wisconsin - Madison) A. G. Akeroyd and CC: PRD 80,
More information12.2 Problem Set 2 Solutions
78 CHAPTER. PROBLEM SET SOLUTIONS. Problem Set Solutions. I will use a basis m, which ψ C = iγ ψ = Cγ ψ (.47) We can define left (light) handed Majorana fields as, so that ω = ψ L + (ψ L ) C (.48) χ =
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 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 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 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 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 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 informationPati-Salam GUT-Flavour Models with Three Higgs Generations
Pati-Salam GUT-Flavour Models with Three Higgs Generations Florian Hartmann in collaboration with Wolfgang Kilian and Karsten Schnitter based on: JHEP 1405 (2014) 064 and arxiv:1405.1901 Universität Siegen
More informationCOLLIDER STUDIES OF HIGGS TRIPLET MODEL
LHC Symposium @ 2011 PSROC Annual Meeting January 26, 2011 COLLIDER STUDIES OF HIGGS TRIPLET MODEL Cheng-Wei Chiang ( ) National Central Univ. and Academia Sinica A. G. Akeroyd and CC: PRD 80, 113010 (2009)
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 informationRG evolution of neutrino parameters
RG evolution of neutrino parameters ( In TeV scale seesaw models ) Sasmita Mishra Physical Research Laboratory, Ahmedabad, India Based on arxiv:1310.1468 November 12, 2013 Institute of Physics, Bhubaneswar.
More information21th. December 2007 Seminar Univ. of Toyama. D6 Family Sym. and CDM at LHC J. Kubo, Y. Kajiyama (Phys. Rev. D )
21th. December 2007 Seminar Univ. of Toyama D6 Family Sym. and CDM at LHC J. Kubo, Y. Kajiyama (Phys. Rev. D75.033001) Plan to talk 1; 2; 2-1); canonical seesaw 2-2); radiative seesaw(ma model) 3; Textures
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 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 informationTHE SEESAW MECHANISM AND RENORMALIZATION GROUP EFFECTS
THE SEESAW MECHANISM AND RENORMALIZATION GROUP EFFECTS M. LINDNER Physik Department, Technische Universität München James-Franck-Str., D-85748 Garching/München, Germany E-mail: lindner@ph.tum.de Neutrino
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 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 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 informationJ. C. Vasquez CCTVal & USM
Maorana Higgses at Colliders arxiv:1612.06840 J. C. Vasquez CCTVal & USM ( Work in collaboration with F. esti and M. emevsek) University of Massachusetts, October 2017 Outline The minimal LR model Decay
More informationFermion Mixing Angles and the Connection to Non-Trivially Broken Flavor Symmetries
Fermion Mixing ngles and the Connection to Non-Trivially Broken Flavor Symmetries C. Hagedorn hagedorn@mpi-hd.mpg.de Max-Planck-Institut für Kernphysik, Heidelberg, Germany. Blum, CH, M. Lindner numerics:.
More informationarxiv:hep-ph/ v1 15 Sep 2000
CU-TP/00-09 Small Violation of Universal Yukawa Coupling and Neutrino Large Mixing arxiv:hep-ph/0009181v1 15 Sep 2000 T. Teshima ) and T. Asai Department of Applied Physics, Chubu University Kasugai 487-8501,
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 informationLepton Flavor and CPV
Lepton Flavor and CPV Alexander J. Stuart 25 May 2017 Based on: L.L. Everett, T. Garon, and AS, JHEP 1504, 069 (2015) [arxiv:1501.04336]; L.L. Everett and AS, arxiv:1611.03020 [hep-ph]. The Standard Model
More informationAlternatives to the GUT Seesaw
Alternatives to the GUT Seesaw Motivations Higher-dimensional operators String instantons Other (higher dimensions, Higgs triplets) Motivations Many mechanisms for small neutrino mass, both Majorana and
More informationNeutrino masses : beyond d=5 tree-level operators
Neutrino masses : beyond d=5 tree-level operators Florian Bonnet Würzburg University based on arxiv:0907.3143, JEP 10 (2009) 076 and arxiv:1205.5140 to appear in JEP In collaboration with Daniel ernandez,
More informationarxiv: v1 [hep-ph] 6 Mar 2014
A predictive model of Dirac Neutrinos OSU-HEP-14-03 Shreyashi Chakdar, Kirtiman Ghosh and S. Nandi Department of Physics and Oklahoma Center for High Energy Physics, Oklahoma State University, Stillwater
More informationSolar and atmospheric neutrino mass splitting with SMASH model
Solar and atmospheric neutrino mass splitting with SMASH model C.R. Das 1, Katri Huitu, Timo Kärkkäinen 3 1 Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie
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 informationS 3 Symmetry as the Origin of CKM Matrix
S 3 Symmetry as the Origin of CKM Matrix Ujjal Kumar Dey Physical Research Laboratory October 25, 2015 Based on: PRD 89, 095025 and arxiv:1507.06509 Collaborators: D. Das and P. B. Pal 1 / 25 Outline 1
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 information+ µ 2 ) H (m 2 H 2
I. THE HIGGS POTENTIAL AND THE LIGHT HIGGS BOSON In the previous chapter, it was demonstrated that a negative mass squared in the Higgs potential is generated radiatively for a large range of boundary
More informationLecture 3. A. Yu. Smirnov International Centre for Theoretical Physics, Trieste, Italy
Lecture 3 A. Yu. Smirnov International Centre for Theoretical Physics, Trieste, Italy 25 Spring School on Particles and Fields, National Taiwan University, Taipei April 5-8, 2012 E, GeV contours of constant
More informationSpontaneous CP violation and Higgs spectra
PROCEEDINGS Spontaneous CP violation and Higgs spectra CERN-TH, CH-111 Geneva 3 E-mail: ulrich.nierste@cern.ch Abstract: A general theorem relating Higgs spectra to spontaneous CP phases is presented.
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 informationarxiv: v1 [hep-ph] 2 May 2017
Scotogenic model with B L symmetry and exotic neutrinos A. C. B. Machado Laboratorio de Física Teórica e Computacional Universidade Cruzeiro do Sul Rua Galvão Bueno 868 São Paulo, SP, Brazil, 01506-000
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 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 informationNeutrinos: Three-Flavor Effects in Sparse and Dense Matter
Neutrinos: Three-Flavor Effects in Sparse and Dense Matter Tommy Ohlsson tommy@theophys.kth.se Royal Institute of Technology (KTH) & Royal Swedish Academy of Sciences (KVA) Stockholm, Sweden Neutrinos
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 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 informationarxiv:hep-ph/ v1 12 Apr 2000 K.S. Babu 1 and S.M. Barr 2
OSU-HEP-00-02 BA-00-19 A Mass Relation for Neutrinos arxiv:hep-ph/0004118v1 12 Apr 2000 K.S. Babu 1 and S.M. Barr 2 1 Department of Physics, Oklahoma State University Stillwater, OK 74078, USA 2 Bartol
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 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 informationProbing B/L Violations in Extended Scalar Models at the CERN LHC A Bottom-up Approach
Probing B/L Violations in Extended Scalar Models at the CERN LHC A Bottom-up Approach Kai Wang Institute for the Physics and Mathematics of the Universe the University of Tokyo Madison, 09/21/2009 J. Shu,T.
More informationDIRAC vs MAJORANA? Neutrinos are the only electrically neutral fermions. ff (quarks, charged leptons) If a fermion is charged, ff
DIRAC vs MAJORANA? Neutrinos are the only electrically neutral fermions If a fermion is charged, ff ff (quarks, charged leptons) Majorana Neutrino: ff = ff, cccccccccccc cccccccccc llllllllllll nnnnnnnnnnnn.
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 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 informationNeutrino Basics. m 2 [ev 2 ] tan 2 θ. Reference: The Standard Model and Beyond, CRC Press. Paul Langacker (IAS) LSND 90/99% SuperK 90/99% MINOS K2K
Neutrino Basics CDHSW m 2 [ev 2 ] 10 0 10 3 10 6 10 9 KARMEN2 Cl 95% NOMAD MiniBooNE Ga 95% Bugey CHOOZ ν X ν µ ν τ ν τ NOMAD all solar 95% SNO 95% CHORUS NOMAD CHORUS LSND 90/99% SuperK 90/99% MINOS K2K
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 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 informationDark Ma'er and Gauge Coupling Unifica6on in Non- SUSY SO(10) Grand Unified Models
Dark Ma'er and Gauge Coupling Unifica6on in Non- SUSY SO() Grand Unified Models Natsumi Nagata Univ. of Minnesota/Kavli IPMU PANCK 2015 May 25-29, 2015 Ioannina, Greece Based on Y. Mambrini, N. Nagata,
More informationUniversity College London. Frank Deppisch. University College London
Frank Deppisch f.deppisch@ucl.ac.uk University College London 17 th Lomonosov Conference Moscow 20-26/08/2015 Two possibilities to define fermion mass ν R ν L ν L = ν L ν R ν R = ν R ν L Dirac mass analogous
More informationarxiv: v1 [hep-ph] 5 Jan 2012
NEUTRINO MASSES FROM R-PARITY NON-CONSERVING LOOPS arxiv:1201.1231v1 [hep-ph] 5 Jan 2012 Marek Góźdź, Wies law A. Kamiński Department of Informatics, Maria Curie-Sk lodowska University, pl. Marii Curie
More informationCombining Pati-Salam and Flavour Symmetries
QFET-015-01 SI-HEP-015-01 Combining Pati-Salam and Flavour Symmetries Thorsten Feldmann, Florian Hartmann, Wolfgang Kilian, Christoph Luhn arxiv:1506.0078v1 [hep-ph] Jun 015 Theoretische Physik 1, Naturwissenschaftlich-Technische
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 information35 years of GUTs - where do we stand?
MPI Heidelberg, November 30 2009 35 years of GUTs - where do we stand? Michal Malinský Royal Institute of Technology, Stockholm in collaboration with Stefano Bertolini and Luca di Luzio SISSA/ISAS Trieste
More informationLeptogenesis with type II see-saw in SO(10)
Leptogenesis wit type II see-saw in SO(10) Andrea Romanino SISSA/ISAS Frigerio Hosteins Lavignac R, arxiv:0804.0801 Te baryon asymmetry η B n B n B n γ = n B n γ Generated dynamically if = (6.15 ± 0.5)
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 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 informationSupersymmetric Seesaws
Supersymmetric Seesaws M. Hirsch mahirsch@ific.uv.es Astroparticle and High Energy Physics Group Instituto de Fisica Corpuscular - CSIC Universidad de Valencia Valencia - Spain Thanks to: J. Esteves, S.
More informationQuarks and Leptons. Subhaditya Bhattacharya, Ernest Ma, Alexander Natale, and Daniel Wegman
UCRHEP-T54 October 01 Heptagonic Symmetry for arxiv:110.6936v1 [hep-ph] 5 Oct 01 Quarks and Leptons Subhaditya Bhattacharya, Ernest Ma, Alexander Natale, and Daniel Wegman Department of Physics and Astronomy,
More informationInvestigating Beyond Standard Model
Investigating Beyond Standard Model Joydeep Chakrabortty Physical Research Laboratory TPSC Seminar, IOP 5th February, 2013 1/35 Standard Model A Brief Tour Why BSM? BSM Classification How do we look into
More informationProton decay theory review
Proton decay theory review Borut Bajc J. Stefan Institute, Ljubljana, Slovenia Lyon, 12 1 Introduction STANDARD MODEL: renormalizable level: accidental B and L conservation (no invariants that violate
More informationTesting Origin of Neutrino Mass at the LHC
王凱 ( ワンカイ ) 東京大学数物連携宇宙研究機構 高エネルギー加速器研究機構理論系つくば, 2008 年 11 月 11 日 Tao Han, Biswarup Mukhopadhyaya, Zongguo Si and KW Phys. Rev. D 76, 075013 (2007) [arxiv:0706.0441 [hep-ph]] Pavel Fileviez Pére, Tao Han,
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 informationUniversity College London. Frank Deppisch. University College London
Frank Deppisch f.deppisch@ucl.ac.uk University College London Nuclear Particle Astrophysics Seminar Yale 03/06/2014 Neutrinos Oscillations Absolute Mass Neutrinoless Double Beta Decay Neutrinos in Cosmology
More informationarxiv: v2 [hep-ph] 7 Apr 2018
Neutrino mixing in SO0 GUTs with non-abelian flavor symmetry in the hidden sector arxiv:803.07933v [hep-ph] 7 Apr 08 Alexei Yu. Smirnov and Xun-Jie Xu Max-Planck-Institut für Kernphysik, Postfach 03980,
More informationPhenomenology of the Higgs Triplet Model at the LHC
Phenomenology of the Higgs Triplet Model at the LHC Andrew Akeroyd SHEP, University of Southampton, UK Higgs Triplet Model (HTM) and doubly charged scalars (H ±± ) The decay channel H 1 γγ and contribution
More informationOverview of theory of neutrino mass and of the 0νββ nuclear matrix elements.
Overview of theory of neutrino mass and of the 0νββ nuclear matrix elements. Petr Vogel, Caltech INT workshop on neutrino mass measurements Seattle, Feb.8, 2010 The mixing angles and Δm 2 ij are quite
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 informationarxiv:hep-ph/ v1 2 Apr 2002
DESY 0-033 NBI-HE-0-0 hep-ph/00407 April 00 Baryogenesis via Lepton Number Violation and Family Replicated Gauge Group arxiv:hep-ph/00407v1 Apr 00 H. B. Nielsen and Y. Takanishi Deutsches Elektronen-Synchrotron
More information