PatiSalam and lepton universality in B decays Julian Heeck Moriond - - PowerPoint PPT Presentation

pati salam and lepton universality in b decays
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PatiSalam and lepton universality in B decays Julian Heeck Moriond - - PowerPoint PPT Presentation

PatiSalam and lepton universality in B decays Julian Heeck Moriond - EW Session - 3/22/2019 based on JHEP 1812 (2018) 103 with Daniele Teresi Neutral current, loop-level SM. LHCb anomaly. C 9 = C 10 Good operator (C 9 = C 10


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SLIDE 1

Pati–Salam and lepton universality in B decays

Julian Heeck Moriond - EW Session - 3/22/2019 based on JHEP 1812 (2018) 103 with Daniele Teresi

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SLIDE 2

Moriond 2019 Julian.Heeck@uci.edu 2

  • Neutral current,

loop-level SM.

  • LHCb anomaly.
  • Good operator (C9 = −C10)
  • Tree-level UV: Z’ or leptoquark.
  • High NP scale = heavy new boson = easy to have.
  • Also look for and di-muons at LHC.

[Capdevila+, ‘17; Altmannshofer+, ‘17; Geng+, ‘17; Ciuchini+, ‘17; D’Amico+, ‘17;...] [Aebischer+, 1810.07698; Altmannshofer+, 1704.05435]

[see David’s talk!]

C9 = −C10

[arxiv.org/list/hep-ph/]

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SLIDE 3

Moriond 2019 Julian.Heeck@uci.edu 3

  • Charged current,

tree-level SM.

  • LHCb, BaBar, Belle.
  • Good operator
  • H+, W’ or leptoquark.
  • Low scale, many constraints: B→Kνν, Bc→τν.

[HFLAV; Bernlochner+, ‘17; Di Luzio+, ‘17;...] [Li+, 1605.09308; Alonso+, 1611.06676]

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SLIDE 4

Moriond 2019 Julian.Heeck@uci.edu 4

  • Charged current,

tree-level SM.

  • LHCb, BaBar, Belle.
  • Good operator
  • H+, W’ or leptoquark.
  • Low scale, many constraints: B→Kνν, Bc→τν.
  • Light (< 100 MeV) sterile neutrino? Evades B→Kνν.
  • r right-handed neutrino!

[He, Valencia, ‘12/’17; Greljo+, ‘18; Asadi+, ‘18; Robinson+, ’18; Bečirević+, ‘16; Azatov+, ‘18] [HFLAV; Bernlochner+, ‘17; Di Luzio+, ‘17;...]

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SLIDE 5

Moriond 2019 Julian.Heeck@uci.edu 5

Leptoquarks?

  • Bosons that couple to

quarks & leptons, e.g.

  • Leads to proton decay!

Impose U(1)B or U(1)e,μ,τ?

  • For B anomalies:
  • Too ad hoc?

Leptoquarks part of GUTs as multiplet partners!

[Review: Doršner+, ‘16] [Barr, Freire ‘90; JH, Hambye, PRL 2018]

L

[see Andrei’s talk!]

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SLIDE 6

Moriond 2019 Julian.Heeck@uci.edu 6

Leptoquarks?

  • Bosons that couple to

quarks & leptons, e.g.

  • Leads to proton decay!

Impose U(1)B or U(1)e,μ,τ?

  • For B anomalies:
  • Too ad hoc?

Leptoquarks part of GUTs as multiplet partners!

[Angelescu+, 1808.08179] [Barr, Freire ‘90; JH, Hambye, PRL 2018] [see Andrei’s talk!]

L

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SLIDE 7

Moriond 2019 Julian.Heeck@uci.edu 7

Pati-Salam

  • Fermions:
  • generates massive
  • sets bound
  • Need extra work to lower and get LFUV.

How about scalar leptoquarks?

[Calibbi+, ‘17; Di Luzio+, ‘17; Blanke, Crivellin, ‘18; Bordone+, ‘18] [Valencia, Willenbrock, ‘94; Smirnov, ‘07/’18] [Pati, Salam, ‘74]

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SLIDE 8

Moriond 2019 Julian.Heeck@uci.edu 8

Pati-Salam

  • Breaking (and NR mass!) via scalars
  • Parity requires and sets
  • Only one (symmetric) coupling matrix!

PS relates couplings of different LQs & to neutrinos!

type-I seesaw no proton decay! type-II seesaw

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SLIDE 9

Moriond 2019 Julian.Heeck@uci.edu 9

Type-II seesaw ↔

  • type-II seesaw

[JH, Teresi, 1808.07492]

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SLIDE 10

Moriond 2019 Julian.Heeck@uci.edu 10

Type-II seesaw ↔

  • can give R(K)!

type-II seesaw [JH, Teresi, 1808.07492]

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SLIDE 11

Moriond 2019 Julian.Heeck@uci.edu 11

Type-II seesaw ↔

  • can give R(K)!
  • μ→e conversion too large, use CP phases to suppress.

type-II seesaw [JH, Teresi, 1808.07492]

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SLIDE 12

Moriond 2019 Julian.Heeck@uci.edu 12

& type-II seesaw

  • R(K) and μ→e fix

neutrino parameters!

  • Fixing :

Should show up in next-gen μ→e!

1σ from nu-fit [JH, Teresi, 1808.07492] normal ordering

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SLIDE 13

Moriond 2019 Julian.Heeck@uci.edu 13

& type-II seesaw

  • R(K) and μ→e fix

neutrino parameters!

  • Fixing :

Should show up in next-gen μ→e!

1σ from nu-fit [JH, Teresi, 1808.07492] normal ordering

Non-trivial, only works for type-II seesaw with normal ordering!

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SLIDE 14

Moriond 2019 Julian.Heeck@uci.edu 14

What about ?

  • Difficult, our S1 LQs couple to NR, not νL.
  • Could use the R2 LQs from the EWSB, but too flexible.
  • Forget neutrino connection and assume one light NR.
  • S3 gives R(K), S1 gives R(D),

same coupling matrix

  • Fixing :
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SLIDE 15

Moriond 2019 Julian.Heeck@uci.edu 15

  • Difficult, our S1 LQs couple to NR, not νL.
  • Could use the R2 LQs from the EWSB, but too flexible.
  • Forget neutrino connection and assume one light NR.
  • S3 gives R(K), S1 gives R(D),

same coupling matrix

  • Fixing :

R(K) R(D)

What about ?

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SLIDE 16

Moriond 2019 Julian.Heeck@uci.edu 16

  • S1 testable in Belle-II:

and at the LHC:

  • here.

Belle II

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Moriond 2019 Julian.Heeck@uci.edu 17

R(K) & R(D) R(K) & R(D) pp → τν pp → S1S1 → tμtμ

[Azatov+, 1807.10745]

pp → ννj

LHC

[CMS-PAS-B2G-16-027] [ATLAS, 1801.06992]

largest LQ coupling

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SLIDE 18

Moriond 2019 Julian.Heeck@uci.edu 18

Conclusions

  • Lepton non-universality in B decays very intriguing.
  • New physics in the form of Z’, W’ or leptoquarks!
  • LQ explanation fits surprisingly nicely into Pati-Salam:

– Required for symmetry breaking & seesaw. – Automatically chiral & no proton decay. – Pati-Salam relates couplings of LQs and seesaw. – Parity relates S3 and S1 couplings.

  • Testable:

L

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SLIDE 19

Moriond 2019 Julian.Heeck@uci.edu 19

Backup

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Moriond 2019 Julian.Heeck@uci.edu 20

Fermion masses

  • Just complex
  • Diagonalization:

with parity relation

  • Adding gives freedom (4HDM) and R2 LQs.

[JH, Teresi, 1808.07492]

[Volkas, ‘95] [Maiezza+, ‘10]

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SLIDE 21

Moriond 2019 Julian.Heeck@uci.edu 21

RGEs

  • The Pati-Salam relations and are broken!
  • RGEs depend strongly on all other particle masses.
  • Heavy NR:

[JH, Teresi, 1808.07492]

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SLIDE 22

Moriond 2019 Julian.Heeck@uci.edu 22

RGEs

  • The Pati-Salam relations and are broken!
  • RGEs depend strongly on all other particle masses.
  • Light NR:

[JH, Teresi, 1808.07492]

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SLIDE 23

Moriond 2019 Julian.Heeck@uci.edu 23

Unification

  • Parity requires at the PS scale. Possible?
  • RGEs depend strongly on all other particle masses.
  • Lowest order:
  • More light states

change this.

[JH, Teresi, 1808.07492]