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The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy of: http://www.symmetrymagazine .org/article/october-2012/w hat-else-could-the-higgs-be

The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

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Page 1: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

The Electroweak Phase Transition within natural GNMSSM models

Presenter: Christopher HarmanSupervisor: Dr. Stephan Huber

University of Sussex

Image courtesy of: http://www.symmetrymagazine.org/article/october-2012/what-else-could-the-higgs-be

Page 2: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

What is supersymmetry?

SUSYSUSYSTANSTAN

SUPERSYMMETRY INVARIANT THEORYSUPERSYMMETRY INVARIANT THEORY

Page 3: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

What is supersymmetry?

SUSYSUSY

STANSTAN

SUPERSYMMETRY INVARIANT THEORYSUPERSYMMETRY INVARIANT THEORY

Page 4: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

What is natural supersymmetry?

FESTIVE EDITIONFESTIVE EDITION

Page 5: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

What is natural supersymmetry?

natural

unnatural

Page 6: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

What is natural supersymmetry?

natural

unnatural excluded

Page 7: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

What is the MSSM?

MSSM: Minimal Supersymmetric Standard Model

Motivation: To address deviations (?) and physics not addressed by the Standard ModelTheory: A type II 2HDM with supersymmetry invariance at the high-scale and soft SUSY broken terms to describe the low energy scales

Page 8: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

What is the NMSSM?

NMSSM: Next-to-MSSM

Motivation: To resolve the μ-problemTheory: Include a singlet chiral superfield into the Higgs sector of the MSSM

Page 9: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

GNMSSM: Generalised NMSSM

Motivation: Include all possible renormalisable terms in the superpotential

What is the GNMSSM?

Not in the scale-invariant NMSSM

Page 10: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 11: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 12: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

The (effective) potential is given by

with CP violating phases ``switched off’’.

It contains the following free parameters

The one loop zero temperature potential

Page 13: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Parameter point scan

Page 14: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Randomly assign a (natural) value

Parameter point scan

Page 15: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Randomly assign a (natural) valueEnsure: 1.No linear term in S at the zero field value2.Zero field minimum and EW broken minimum are degenerate (CHOICE!)

Parameter point scan

Page 16: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Randomly assign a (natural) valueEnsure: 1.No linear term in S at the zero field value2.Zero field minimum and EW broken minimum are degenerate (CHOICE!)Record parameter points satisfying certain criteria, e.g.: stable potential, physical masses.

Parameter point scan

Page 17: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

At tree level

At tree level, we find

but this is insufficient for a 125 GeV Higgs…

… go to one-loop level!

Page 18: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 19: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 20: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Parameter point scan

Page 21: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Choose a specific stop structure:1.No gauge eigenstate mixing:2.Stop soft mass deviation:

Parameter point scan

Page 22: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Choose a specific stop structure:1.No gauge eigenstate mixing:2.Stop soft mass deviation:Assign a value to Δm3 and scan over natural values of mQ3 until a 125 GeV Higgs is obtained

Parameter point scan

Page 23: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Parameter point scan (two distinct potential shapes)

TYPE 1

Tree

1 loop

Page 24: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Parameter point scan (two distinct potential shapes)

TYPE 1

1 loop

Page 25: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Parameter point scan (two distinct potential shapes)

TYPE 2

Tree

1 loop

Page 26: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Parameter point scan (two distinct potential shapes)

TYPE 2

1 loop

Page 27: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 28: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 29: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

One loop finite temperature potential

Include to the potential the following term:

We implement this into our program and obtain values for the critical temperature and critical VEV by numerical means

Page 30: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

One loop level (finite temperature)

We implement this into our program and obtain values for the critical temperature and critical VEV by numerical means Tree

1 loop (0T)1 loop (finite T)TYPE 1

TYPE 2

Page 31: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 32: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 33: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Aim of the project

Page 34: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Outlook

CONCLUSIONS:•Can have a 125 GeV Higgs in the GNMSSM•EWPT is found to be rather strongly first order for around 200 natural parameter points

FUTURE WORK:•Relax some of our choices:– Tree-level minima degeneracy (Aλ choice);– No stop mixing (At choice);– Stop soft mass deviation (Δm3 choice)

•Repeat the analysis

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Thank you!

S. Martin, A SUSY Primer: http://arxiv.org/abs/hep-ph/9709356U. Ellwanger, The NMSSM: http://arxiv.org/abs/arXiv:0910.1785G. Ross et al., The GNMSSM at one loop: fine tuning and phenomenologyG. Anderson and L. Hall, The Electroweak phase transition and baryogenesis

Page 36: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

• Gauge eigenstate basis:

• Mass eigenstate basis:CP-even partCP-even part CP-odd partCP-odd part

Charged partCharged part

The tree-level potential

Page 37: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

One-loop level (zero temperature)Green – Exact solution with degenerate stopsRed – Naïve solution with non-degenerate stops

Page 38: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

One-loop level (finite temperature)

Include to the potential the following term:

Piece-wise analytic function can be constructed

Page 39: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Finite temperature potential (analytic)

Page 40: The Electroweak Phase Transition within natural GNMSSM models Presenter: Christopher Harman Supervisor: Dr. Stephan Huber University of Sussex Image courtesy

Parameter scan statistics

Models with an unstable singlet potential only: 17.9477 %Models with at least one unphysical mass only: 6.40353 %Models with both of the above issues: 73.7124 %Models with none of the above issues: 1.93641 %

Runs: 20192 Successes: 20192