SU(5)-type unification of Yukawa couplings of fermions in MSSM - - PowerPoint PPT Presentation

su 5 type unification of yukawa couplings of fermions in
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SU(5)-type unification of Yukawa couplings of fermions in MSSM - - PowerPoint PPT Presentation

SU(5)-type unification of Yukawa couplings of fermions in MSSM Mateusz Iskrzy nski University of Warsaw in collaboration with Mikolaj Misiak, Ulrich Nierste, Andreas Crivellin The project International PhD Studies in Fundamental Problems


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SU(5)-type unification of Yukawa couplings of fermions in MSSM

Mateusz Iskrzy´ nski

University of Warsaw

in collaboration with Mikolaj Misiak, Ulrich Nierste, Andreas Crivellin

The project ”International PhD Studies in Fundamental Problems of Quantum Gravity and Quantum Field Theory”is realized within the MPD programme of Foundation for Polish Science, cofinanced from European Union, Regional Development Fund Planck 2013: From the Planck Scale to the Electroweak Scale Bonn, 21.05.2013

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MSSM: From the GUT scale to the Electroweak Scale

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Problem’s anatomy in SU(5)

In SM and MSSM the fermion masses are independent parameters and are given by 3 Yukawa matrices: Y u → mu, mc, mt Y d → md, ms, mb Y e → me, mµ, mτ In SU(5) Supersymmetric Grand Unified Theory the symmetry requires: Yd = Ye, Ys = Yµ, Yb = Yτ

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Yukawa unification

Succesful unification of bottom and tau Yukawa couplings: tan β = 10, M1/2 = m0 = 600GeV , Ade = 0

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Yukawa unification

Unsuccesful unification of strange and mu Yukawa couplings: tan β = 10, M1/2 = m0 = 600GeV , Ade = Au = 0

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Yukawa unification - Solution 1 - fix GUT structure

Change the boundary condition at the high scale

◮ non-minimal representations of Higgs superfields ◮ correction O(1) from higher-dim. operators

◮ original idea accompanying GUTs in ’70s ◮ many modern treatments: 0903.2793, 1009.6000, 1101.5423,

1109.3396, 1211.0516

◮ also with other mechanisms: 1211.6529, 1202.4012

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Yukawa unification - Solution 2

Manipulate the boundary condition between SM and MSSM - play with treshold corrections ’06 Diaz-Cruz, Murayama, Pierce, arXiv: hep-ph/0012275 Our analysis:

◮ full 1-loop chirality changing treshold corrections in MSSM

(implemented as modification to Softsusy 3.3.5 Allanach,

hep-ph/0104145 )

◮ simpler ansatz ◮ no tension with flavour observables - heavy gluino (calculated with

SUSY Flavor 2.02 Crivellin, Rosiek, Chankowski, Dedes, Jaeger, Tanedo,

1203.5023)

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Yukawa unification - Solution 2

Manipulate the boundary condition between SM and MSSM - play with treshold corrections (dotted - running for unadjusted lower boundary condition)

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Relevant parameters

Soft-supersymmetry breaking terms in MSSM: Lsoft ∋ ˜ qAu˜ uhu + ˜ qAd ˜ dhd +˜ lAe˜ ehd

Yukawa couplings can be unified within MSSM

with big diagonal A terms making MSSM vacuum metastable

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Dependencies on MSSM parameters

Ad

ii can be used to adjust the magnitude of treshold correction to

achieve unification for given values of other parameters Y d

ii =

md

i − ΣdLR / Y

(αsm˜

gAd ii, m˜ qi, m˜ di)

vd[1 + tan β · ǫd(µ, M1, M2, m˜

qi, m˜ di)]

  • A. Crivellin, L. Hofer, J. Rosiek, JHEP 1107 (2011) 017 [arXiv:1103.4272]
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Strange quark and muon

Yukawa couplings can be unified within MSSM with big A terms

for the 2nd family the shift has to be the biggest

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Positive impact on (g − 2)µ

tan β = 10, M1/2 = m0 = 600GeV , µ ∈ [−1000, −200]

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Relevant stability condition

Along the direction in space of scalar fields of MSSM where |H1| = | ˜ sL| = |˜ sR| a deeper, charge and color breaking minimum develops if Ad

22 is of the

  • rder considered here. The absolute stability conditions

(given by Casas, Lleyda, Munoz, arXiv: hep-ph/9507294 ) Aii Yii ˜ m < O(1) are violated: → A22 Y22 ˜ m2 (QEWSB) ≈ 2 ∗ 102

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Metastable but durable

The decay time of the correct MSSM vacuum were longer than the age

  • f the Universe if

A22 ˜ m < 1.75

Borzumati, Farrar, Polonsky, Thomas Nuclear Physics B 555 (1999) 53-115:

is still satisfied in the considered model of Yukawa unification.

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Conclusion

Yukawa couplings can be unified within MSSM

with big diagonal A terms making MSSM vacuum metastable

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Unavoidable?

Could we unify Ys and Yµ satisfying absolute stability bound, for which Ade/ ˜ m 0.01 ? Y d

ii =

md

i − ΣdLR / Y

(αsm˜

gAd ii, m˜ qi, m˜ di)

vd[1 + tan β · ǫd(µ, M1, M2, m˜

qi, m˜ di)]

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Just treshold corrections

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Impact of squark masses

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The actual scan

tan β = 40, M1/2 = m0 = 600GeV , Ade = 0

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B to s gamma unaffected by Ade22

tan β = 10..40, M1/2 = m0 = 600GeV

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Dominant corrections in complete form

i - generation Σ, ǫ - self-energies mqi = vqY qi + Σq,LR

ii

(Y q) mdi = vdY di + Σ /

Y ii + vuY diǫd i + O( v2 MSUSY 2 )

Y d

ii =

md

i − ΣdLR / Y

vd[1 + tan β · ǫd]

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Down quark and electron 1

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Down quark and electron 2

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Down quark and electron 3