CORFU HDMs. symmetry The Inert Model Various vacua Today= Inert phase Thermal evolutions Z 2

Transcription

1 CORFU HDMs Z 2 symmetry The Inert Model Various vacua Today= Inert phase Thermal evolutions Maria Krawczyk University of Warsaw I. Ginzburg, K. Kanishev (Novosibirsk University), D.Sokołowska, G. Gil, B. Gorczyca (University of Warsaw)

2 Brout-Englert-Higgs mechanism Spontaneous breaking of EW symmetry SU(2) x U(1) U(1) QED Standard Model Doublet of SU(2): Φ= (ϕ +,v+h+iζ) Τ Masses for W +/, Z (tree ρ =1), no mass for the photon Fermion masses via Yukawa interaction Higgs particle H SM - spin 0, neutral, CP even couplings to WW/ZZ, Yukawa couplings to fermions mass selfinteraction unknown

3 Brout-Englert-Higgs mechanism Spontaneous breaking of EW symmetry SU(2) x U(1)? Two Higgs Doublet Models Two doublets of SU(2) (Y=1, ρ =1) - Φ₁, Φ₂ Masses for W +/, Z, no mass for photon? Fermion masses via Yukawa interaction various models: Model I, II, III, IV,X,Y,... 5 scalars: H+ and H- and neutrals: - CP conservation: CP-even h, H & CP-odd A - CP violation: h 1,h 2,h 3 with undefinite CP parity* Sum rules (relative couplings to SM χ)

4 2HDM Potential Lee'73, Haber, Gunion, Glashow, Weinberg, Paschos, Despande, Ma, Wudka, Branco, Rebelo, Lavoura, Ferreira, Barroso, Santos, Bottela, Silva, Diaz-Cruz, Grimus, Ecker, Ivanov, Ginzburg, Krawczyk, Osland, Nishi, Nachtmann, Akeroyd, Kanemura, Kalinowski, Grządkowski,Hollik, Rosiek.. V = λ 1 (Φ₁ Φ₁)²+λ₂(Φ₂ Φ₂)²+λ₃(Φ₁ Φ₁)(Φ₂ Φ₂) + λ₄(φ₁ Φ₂)(Φ₂ Φ₁)+ [λ₅(φ₁ Φ₂)²+h.c] + [(λ₆(φ₁ Φ₁)+λ₇(Φ₂ Φ₂))(Φ₁ Φ₂)+h.c] -m²₁₁(φ₁ Φ₁)-m²₂₂(Φ₂ Φ₂)-[m²₁₂(Φ₁ Φ₂)+h.c. m²₁₂(φ₁ Φ₂)+h.c.] Z₂ symmetry transformations: Φ₁ Φ₁ Φ₂ - Φ₂ Φ₁ -Φ₁ Φ₂ Φ₂ Hard Z₂ symmetry violation: λ₆, λ₇ terms Soft Z₂ symmetry violation: m²₁₂ term Explicit Z₂ symmetry in V: λ₆, λ₇, m²₁₂=0 (Re m²₁₂=µ²)

5 Inert Model or Dark 2HDM Ma'78 Barbieri'06 Z 2 symmetry under Φ₁ Φ₁ Φ₂ - Φ₂ both in L and in vacuum Inert Model Today <Φ₁ >= v <Φ 2 >= 0 Φ₁ as in SM (BEH( BEH), with Higgs boson h (SM-like) Φ₂ - no vev,, with 4 scalars (no Higgs bosons!) no interaction with fermions (inert( doublet) Conservation of the Z 2 symmetry; only Φ₂ has odd Z 2 -parity The lightest scalar a candidate for dark matter (Φ dark doublet with dark scalars) ).

6 We are in the Inert phase Φ₁ Φ S Higgs doublet S Φ₂ Φ D Dark doublet D Two Z₂ transformations: S: Φ S - Φ S Φ D Φ D SM SM D: Φ S Φ S Φ D - Φ D SM SM Other vacua? Where we were before?

7 Lagrangian

8 Vacua for the potential with explicit Z symmetry and real parameters 2 Finding extrema: V / Φ = 0 Φ = <Φ> < Finding minima global minimum = vacuum Positivity (stability) constraints Ginzburg, Kanishev, MK, Sokołowska'09 Extremum fulfilling the positivity constraints with the lowest energy = vacuum

9 Possible vacuum states (V with explicit Z 2 ) The most general vacuum state EWs EWs v S, v D, u, - real, 0 v =v 1 +v 2 +u 2 = (246 GeV) 2 u = v D =v S = 0 Inert I 1 u = v D = 0 Inert-like I 2 u = v S = 0 Mixed M u = 0 Charge Breaking Ch u 0 0 v D =0

10 Various vacua on (λ(, λ ) plane 4 5 Positivity constrains on V: X= λ 1 λ 2 +λ 3 >0 λ 4 ± λ 5 > - X Inert and Inert-like 2 Y = M H+ 2/v 2 Mixed Charge Breaking Ch Note the overlap of the Inert with M and Ch!

11 TODAY 2HDM with explicit S (Z 2 ) symmetry Φ S Φ S Φ D - - Φ D Model I (Yukawa int.) Charged breaking phase? photon is massive, el.charge is not conserved... no Neutral phases: Mixed M ok, many data, but no DM Inert I1 OK! there are some data Inert-like I2 no, all fermions massless, no DM

12 Inert Model (Dark 2HDM) vs data Ma..' 78, Barbieri.. ' 2006 Exact (D)Z₂ symmetry in L and in vacuum D-parity: odd is only Φ D Φ S Nonzero vev has only doublet Φ S (Higgs doublet) only it couples to fermions (Model I) SM-like Higgs boson h M 2 = m 2 = λ h 11 1 v 2 Φ D Zero vev for ΦD (scalar doublet) and no Yukawa int. Four scalars with odd Z₂-parity (dark scalars D) The lightest dark scalar - stable

13 Dark scalars D = H+,H-,H,A Masses D couple to V = W/Z (eg. AZH, H W+H), + not to DV V! Selfcouplings DDDD proportional to λ 2 Couplings between Higgs boson h and D proportional to M 2 + m 2 /2 D 22

14 Intert Model dark scalar masses Y = M H+ using X (positivity) and Y = M 2/v 2 H+ 2 2/v here H+ the heaviest here H is the dark matter candidate (λ( 5 < 0)

15 Testing Inert Model To consider properties of SM-like h (light and heavy) properties of dark scalars (produced only in pairs!) DM candidate Colliders signal/constraints Barbieri et al '2006 for heavy h Cao, Ma, Rajasekaren' 2007 for a light h

16 Dark 2HDM: LEP II exclusion: H vs A Lundstrom et al LEP II + WIMP = 200 GeV M h M A - M H > 8 GeV

17 Inert Model: constraints LEP+DM LHC E. Dolle, S. Su, [hep-ph] LEP (exclusion and EW precision data) + relic density using MicroOMEGA/CalCHEP S=H Su, CERN, August 2009

18 Other analysis (IDM) Gustafsson et al.2007: striking DM line signals -promising features to search with GLAST Mass of: H = GeV, H+ = 170 GeV, A = GeV, h = 500 and 120 GeV Honorez, Nezri, Oliver, Tytgat H as a perfect example or arcgetype of WIMP within reach of GLAST (FERMI) Here mass of h = 120 GeV, mass H+ close to A = GeV C. Arina, F-S Ling, M. Tytgat 2009 IDM&iDM or the inert doublet Model and inelastic dark matter Mass H=10 GeV and 535 GeV 50 TeV! (DAMA data)

19 Evolution of the Universe different vacua in the past Ginzburg, Ivanov,Kanishev 2009 Ginzburg, Krawczyk, Sokołowska 2010 We consider 2HDM with an explicit Z 2 symmetry assuming that today the Inert Model is realized. Yukawa interaction Model I all fermions couple only to Φ S

20 Possible neutral extrema (u=0): Inert B u=0 N a true vacuum with the minimal energy

21 Energy difference I 1 -I 2 : I 1 -M I 2 -M For M vacuum to exist: (1-R)(1+R)>0 1-R>0

22 Thermal corrections of V Matsubara method (temperature T>> m 2 ) -only quadratic (mass) parameters change with T Positivity condition: EW coupling constant with T different phases possible

23 Phase transitions from the EW symmetric phase The phase diagram The evolution parameters to the present INERT phase

24 vacua I min I 1 I 2 min

25 R>1 Mixed vacuum impossible

26 0<R<1

27 -1<R<0

28 Masses of scalars vs T2 Mh=120 GeV MH+=110 M A =68 M H =60 ray VIII h H+ A H Φ S Φ D Inert M Inert-like EWs

29 Masses of scalars vs T Mh=120 GeV MH+=110 h M A =68 M H =60 H+ A Φ S ray V H Φ D Inert Inert-like EWs

30

31 Without fermions in evolution parameter c1

32 Non-restoration of EW symmetry c 1 or c 2 < 0

33 excluded if DM neutral! DM matter may appear later.. Conclusions Intert Model in agreement with present data soon tests at FERMI and LHC What was in the Past? Various scenarios Can we find clear signals?