gauged b l leptogenesis
play

Gauged B-L Leptogenesis Shaaban Khalil Center for Fundamental - PowerPoint PPT Presentation

Gauged B-L Leptogenesis Shaaban Khalil Center for Fundamental Physics Zewail City of Science and Technology Introduction The recent observations indicate that the asymmetry between number density of baryon ( ! " ) and of anti-baryon ( !


  1. Gauged B-L Leptogenesis Shaaban Khalil Center for Fundamental Physics Zewail City of Science and Technology

  2. Introduction • The recent observations indicate that the asymmetry between number density of baryon ( ! " ) and of anti-baryon ( ! # " ) of the universe is given • In the SM, the baryon asymmetry is $ " ≈ &' ()* , which is too small to account for the observed baryon asymmetry. • Leptogenesis through the decay of a heavy singlet neutrino is considered as the best scenario for understanding the observed baryon asymmetry of the Universe. • In this mechanism, the lepton asymmetry Y L can be converted to baryon asymmetry Y B via the electroweak sphaleron according to this relation , $ " = , − & $ . * 0 1 23 0 4 / = )) 0 1 2&5 0 4 , and 0 1 is the number of fermions and 0 4 is the number of Higgses.

  3. • The lepton asymmetry is given by • Lepton asymmetry arises due to interference between tree & loop contributions • Thus • Therefore, the necessary condition for leptogenesis is • Due to the unitarity of UMNS, leptogenesis does not depend on low energy phase appears in the leptonic mixing matrix. If the matrices R and M R are real the ! 1 =0.

  4. • Finally, the baryon asymmetry is given by $ $ ) & * ∗ ≈ &- %. ( ) & ! " = $%& ! ' = $%& ( The coffecient ( parametrize the wash out effect due to the inverse decay and the scattering processes. It depends on the ratio / = 0 12& /4 ; ( ( ~ 1/K). • For 6 12& ~ &- &- 789 ⇒ ( ~; & and ! " ≈ &- %. ) & • For 6 12& ≪ 6 12. , 6 12> ;(&- &> ) • Thus, the required baryon asymmetry can be obtained. • In this case, the energy scale involved in a successful application is in the range 10 9 to 10 13 GeV, which renders the idea impossible to verify experimentally

  5. TeV scale Leptogenesis • We now consider TeV scale Seesaw mechanism. In this case, after the TeV scale symmetry (e.g., B−L) breaking, the neutrino mass matrix is given by • With m D = Y ν v 2 , M N = Y N v 1 ʹ. The neutrino masses are • Therefore, if M N ∼ O(1) TeV, the light neutrinos ν ℓ mass can be of order one eV if the Yukawa coupling Y ν ~ 10 −6. • This small coupling is of order the electron Yukawa coupling, so it is not quite unnatural.

  6. In TeV scale type I seesaw, ! " ~ $ %& '( • and ) * ~ $ +,- , the lepton asymmetry can be written as Thus, for /) = ) 1 − ) % ~ $(%& '4 ), the required baryon asymmetry can be • obtained. Based on this fine tuning, a “Resonant Leptogenesis” is defined. •

  7. Inverse Seesaw Mechanism • # and In this class of models, the SM is extended with three right-handed neutrinos, ! " three singlet fermions $ # . • The Lagrangian of neutrino masses, in the flavor basis, is given by: 3 4 + h. c. ) + 9 : ̅ + , - . + 0 1 2 4 3 4 ℒ = (( ) ̅ - .

  8. Leptogenesis with Inverse Seesaw

  9. Gauged B − L Leptogenesis • " # with B − L = 1 implies In supersymmetry, the addition of the singlet superfield ! a fermion " # and a scalar $ " # . After the B−L symmetry breaking by the VEVs < & ',) > = , ',) , a bilinear • ) $ 0 $ 0 is obtained and it is given by coupling - ./ " . " / 5 + 4 " , 3' 7′ ∗ ) = −, 3' 4 " - 1 ) = 0 so that the off-diagonal elements of sneutrino $ " # • Here, we assume that - 1 mass matrix, in the ($ 0 , $ 0∗ ) basis, vanish. " . " . " #∗ are mass eigenstates with mass squared Therefore, $ " # , $ • ∗ < 1 = + > ) + ) BCD2F ' < 1 ? 1 @ < A3 They have lepton numbers G = ∓I respectively. Moreover, if cos 2θ is negative, • " # can be lighter than " # . $ This is the crucial assumption of our proposal. •

  10. The Lagrangian, in flavor eigenstates, relevant for our analysis is given by • The Lagrangian in mass eigenstate is given by • Where • The four-component Majorana spinors are defined as ( , assuming the mass hierarchy Now, we consider leptogenesis by ! " → $ % & • ! ' ) !" ≪ ) !+,- . We assume that only the lightest B − L neutralino $ ≡ $ " and ( are lighter than ! " , and satisfy the relation sneutrino of the third generation & ! - 2 < ) ! " . / 0 + ) & ! - ( carries lepton number, the decay: Due to the fact that 4 ! = 6 , & • ! - ( violates lepton number. ! " → $ & ! -

  11. • ' decay CP asymmetry of ! " → $ % ! & processes is generated by the interference between tree and one- loop level diagrams of vertex and self-energy correction • ' decay processes is generated by the interference CP asymmetry of ! " → $ % ! & between tree and one-loop level diagrams of vertex and self-energy correction • It is defined as • The decay rate ( at one-loop level is given by Where the phase space integral of two-body decay ) * is given by

  12. • ' decay has the structure: We found that the CP asymmetry ! " → $ % ! & where we assumed diagonal right-handed mass matrix. One finds ( "& ~*+, - ≪ " , as 5 !" required by out-of equilibrium condition: ( ( ! " → $ % ' ) < 0(2 = ") , for 2 = ! & 6 . Also ( && ~789 :~" , which leads to a large CP asymmetry. This situation is realized if the mixing matrix ( is almost diagonal. • In our model, baryon asymmetry is obtained through the following procedure: ' decay generates % ' asymmetry ; ∆% 1. ! " → $ % ! & ! & ! . ' decays into (s)lepton by Dirac Yukawa couplings, soft SUSY breaking A-term 2. % ! & and = -term, and resulting (s)lepton asymmetry ; ∆>(∆? @) is obtained by solving the Boltzmann equations. 3. Sphaleron converts total lepton asymmetry ; > = ; ∆> + ; ∆? @ to baryon asymmetry ; A .

  13. Boltzmann Equations The Boltzmann equation describing the evolution of ! " is • ! " is the number of particle in a comoving volume element, which is given by the ratio of # " and the entropy density s .

  14. Enough baryon asymmetry is obtained.

  15. Conclusion We have shown that a successful TeV scale leptogenesis can take place in • gauged B − L supersymmetric model. In this model, if the right-sneutrino bilinear term is absent, then the lightest • $ is lighter than " % and sneutrino is assigned a lepton number. Therefore if ! " # " & is almost diagonal, a large lepton asymmetry can be scalar mass matrix of ! generated by B−L neutralino interactions of O (1) couplings ' ()* and/or + " $ for the decay " % → - ! $ . through the one-loop exchange of " # " # $ is transmitted into asymmetry of lepton and slepton This asymmetry of ! " # • through the Yukawa coupling, trilinear coupling, and μ-term, and sphaleron converts lepton asymmetry to baryon asymmetry.

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend