Left-Right Models Radiatively Broken by a Doublet Nathan Papapietro - PowerPoint PPT Presentation

Left-Right Models Radiatively Broken by a Doublet Nathan Papapietro University of Alabama SUSY 2015, AUG 23-29 In collaboration with Nobuchika Okada (University of Alabama) Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Breaking Path The existing gauge symmetries at low energies, SU (3) c × U (1) em , are vector-like. At higher energies ( µ ∼ Λ SM ) there is a parity violation in nature due to the axial nature of SU (2) L . Gauge parity can be restored at even higher energies using Left-Right Models, first proposed by Pati and Salam 1 SU (4) c × SU (2) L × SU (2) R We choose to start at: SU (3) c × SU (2) L × SU (2) R × U (1) B − L → SU (3) c × SU (2) L × U (1) Y Which is broken down into the Standard Model. 1 Pati, J. C. and Salam, A., Phys. Rev. D 10, 275 (1974) Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Particle Contents To achieve realistic fermion masses, a 2nd higgs bidoublet is added. SU (3) c SU (2) L SU (2) R U (1) B − L 3 2 1 1 / 3 Q ¯ Q c 3 1 2 − 1 / 3 1 2 1 − 1 (1) L L c 1 1 2 1 h 1 2 2 0 h ′ 1 2 2 0 The superpotential is W = Y q QhQ c + Y ′ q Qh ′ Q c + Y e LhL c + Y ′ e Lh ′ L c + α Tr hh + α ′ Tr h ′ h ′ + β Tr hh ′ + h . c . The soft mass terms are L c | ˜ L | ˜ Q c | ˜ Q | ˜ V soft = m 2 L c | 2 + m 2 L | 2 + m 2 Q c | 2 + m 2 Q | 2 + m 2 h | h | 2 + m 2 h ′ | h ′ | 2 + O ( hh ′ ) (2) In order to achieve radiative breaking, there needs to be a soft mass splitting at some higher energy, meaning this model does not have matter parity symmetry, only gauge parity symmetry. Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Breaking Mechanism Doublets were initially proposed 2 , but after the seesaw was introduced 3 triplet models were introduced to achieve a seesaw mechanism without R-Parity breaking. However to achieve LRM breaking without Q em violation, R-Parity has to be broken as well 4 leading to nonzero VEV of � ˜ L c � = v R 2 . √ m 2 ˜ ˜ N c N c † g 2 BL Figure: Soft mass insertions in D-term corrections must be larger than F-term and Gaugino corrections 2 Mohapatra, R. N. and Pati, J. C., Phys. Rev. D 11, 2558 (1975). ,Senjanovic, G. and Mohapatra, R. N., Phys. Rev. D 12, 1502 (1975) 3 Minkowski, P., Physics Letters B 67, 421 (1977) 4 Kuchimanchi, R. and Mohapatra, R. N., Phys. Rev. D 48, 4352 (1993) Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Soft Lepton Mass RGEs 8 π 2 dm 2 ˜ L | 2 � � L i � | Y ijh m 2 L i + m 2 j + m 2 − g 2 BL Tr [ Q BL m 2 ] d ln µ = ˜ ˜ h L c j , k − 4 g 2 BL M 2 BL − 3 g 2 L M 2 L (3) 8 π 2 dm 2 ˜ L c L | 2 � � � | Y ijh m 2 L i + m 2 j + m 2 + g 2 BL Tr [ Q BL m 2 ] d ln µ = i ˜ ˜ L c h j , k − 4 g 2 BL M 2 BL − 3 g 2 R M 2 R The soft slepton mass runnings at one-loop can easily be derived. The U (1) B − L charge dictates sign of the trace: 3 � � � g 2 � Q BL m 2 � 2 g 2 m 2 Q i − m 2 i − m 2 L i + m 2 = . (4) BL Tr BL ˜ ˜ ˜ ˜ Q c L c i i We only need a single large left handed scalar quark doublet to be large which would dominate over even the gaugino masses. Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Soft Quark Mass RGEs Similar to lepton sector, they get additional gluino term. Due to the large top Yukawa, heavy generations run the risk of running negative as well (breaking electromagnetism). This can be avoided by large gluino mass. Q = 2 | Y q | 2 � � m 2 Q + m 2 Q c + m 2 h + m 2 β m 2 ˜ ˜ h ′ ˜ (5) − 4 BL + 1 L − 16 9 g 2 BL M 2 3 g 2 BL Tr [ Q BL m 2 ] − 3g 2 L M 2 3 g 2 3 M 2 3 Qc = 2 | Y q | 2 � � m 2 Q + m 2 Q c + m 2 h + m 2 β m 2 ˜ ˜ h ′ ˜ (6) − 4 BL − 1 R − 16 9 g 2 BL M 2 3 g 2 BL Tr [ Q BL m 2 ] − 3g 2 R M 2 3 g 2 3 M 2 3 With 3 � � � g 2 Q BL m 2 � 2 g 2 m 2 Q i − m 2 i − m 2 L i + m 2 � BL Tr = . (7) ˜ ˜ ˜ ˜ BL Q c L c i i Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Inputs µ GUT = 10 16 GeV and the breaking is around 7 TeV Yukawas and g y , for one heavy generation, were ran from low energy with θ R ≈ 55 ◦ . The couplings are very sensitive to θ R Higgs doublets set at 5 TeV but have minimal influence in runnings Values at GUT Scale: Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Breaking Relations 2 M L � 1 5 � 10 7 Ln � Μ � 6 8 10 12 14 16 � 5 � 10 7 � 1 � 10 8 g Y = g R sin θ R M W R = 1 2 g R v R tan θ R = 2 g BL M Z R = 1 � (8) g R 4 g 2 BL + g 2 2 v R R Y W = Y BL − ( T 3 ) R M A Y = 0 2 Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Tau Lepton constraint and Low Energy R + g R v BL L ⊃ ˜ M ± R λ + R λ − E c λ − √ R + h . c . (9) 2 L ⊃ M ξ + λ − R + h . c . (10) The multiplet has an uneven number in hypercharge= ± 1. There is an orthogonal mode present after the LR breaking. In order to keep the tau lepton from having too large of a mixing angle and exceeding bounds, ˜ M ± R >> M W R . Leaving δ Γ ττ ∼ 10 − 2 Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Neutrino Masses � − 8 m 2 Lc We define the VEV to be v R = BL ) ∼ 20 TeV ( g 2 R + g 2 M W R ∼ 4 . 6 TeV and M Z R ∼ 8 . 3 TeV The mass matrix after the LRM breaking is   M R 0 g R v R M ν c , ˜ R = 0 M BL g BL v R (11) λ BL , ˜ λ 3   g R v R g BL v R 0 We still get a heavy neutrino but after EW breaking we can still induce a light neutrino spectrum via see-saw. m ν ∼ | ˜ Y L | 2 ˜ v 2 u (12) (2 M ν c ) Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Quark Masses Down Quark sector to be a diagonalized matrix M u = D u . Rotate up quark mass to get a diagonalized mass matrix V † km M d V km = D d . After EWSB 1 m u = √ Y q v u 2 1 m ′ Y ′ q v ′ √ u = u 2 Now quark mass matrices can now be expressed as M u = m u + m ′ u = D u (13) M d = cm u + c ′ m ′ u = V km D d V † km v u and c ′ = v ′ Where c = v d u . d v ′ In general, there can be Left and Right KM matrices to rotate the quarks. Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet

Conclusions The Left-Right Models offer great parity restoring phenomnology at higher energies Minimal LRMs without triplets can be broken via right-handed sneutrino radiatively. Due to tau lepton constraint, a very heavy squark is needed. Small neutrino masses can still be produced via gaugino mixings Some fine tuning is needed Nathan Papapietro Left-Right Models Radiatively Broken by a Doublet