Seesaw for the Higgs boson Xavier Calmet Université Libre de Bruxelles.
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Transcript of Seesaw for the Higgs boson Xavier Calmet Université Libre de Bruxelles.
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Seesaw for the Higgs boson
Xavier Calmet
Université Libre de Bruxelles
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Outline
• Review the motivations for physics beyond the standard model.
• What do we know for sure? • Some minimal modifications of the Standard Model
can address these issues• Modification of short distance physics• Modification in the Higgs sector• A gateway to new physics• Conclusions
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Motivations for new physics
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Guiding principles for physics beyond the SM
• Guiding principles for model building have changed.
• Till ‘03 or so hierarchy and naturalness were the main problems to address: why is the weak scale so small compared to the Planck scale and why is the Higgs boson’s mass stable under radiative corrections?
• Indeed if quantum field theories are only an “effective tool” (Wilsonian approach) one has to explain small numbers!
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Guiding principles for physics beyond the SM after 2003
• Post landscape era: fine-tuning is allowed ( or required: anthropic or statistical arguments).
• More important we have experimental evidence that the hierarchy and naturalness problems are not necessarily valid guidance principles:
• Hints from the cosmological constant: not zero and small: unnatural (but observed!!). Effective theories argument would imply new physics at 0.001 eV! No sign of it!
• Next surprise: light Higgs and no SUSY (or little Higgs)?
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• Personal point of view: within the framework of a renormalizable quantum field theory, fine-tuning or hierarchy problems make no sense: a parameter is measured at some scale and one can compute its running.
• So what is the meaning of small or big? It’s an experimental question.
• There may be an esthetic reason against the Higgs: only fundamental scalar?
• But main issue is the negative squared mass: it’s never free to break a symmetry.
• We can hope that the LHC will reveal the mechanism that triggers the Higgs mechanism.
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What do we know for sure?
• Two experimental facts:
• There is dark matter.
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What do we know for sure?
• Two experimental facts:
• There is dark matter.
• Most probably dark energy exits as well.
• Mathematical consistency of the standard model implies that effectively there is a scalar degree of freedom in the standard model (or S matrix is non-perturbative)
• Unification of gravity and quantum mechanics implies a minimal length in nature (see last year talk).
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New picture of the Universe
From astro-ph/0609541(J. R. Primack)
SM
Extended Higgs sector
Minimal length
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How to implement these facts in the Standard Model?
• Minimal length: modify spacetime at short distance: one option is a noncommutative spacetime.
• What are the physical consequences? New insight for the cosmological constant.
• What about the electroweak symmetry breaking: extend the Higgs sector.
• Quite natural to expect that dark matter couples to the Higgs boson, if not it will be very difficult to ever produce it in a collider.
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Gravity on noncommutative spaces
• Hypothesis: is a constant of nature and it has the same value in every coordinate frame.
• Well if that is the situation, what are the coordinate transformations allowed by the NC algebra:
• Let us consider the transformations: and study the NC algebra:
• It is invariant iff
• The solutions are:
• They form a subgroup of 4-vol. preserving coord. transf.
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• If there is an expansion in the action must take the form:
• When we vary the action with respect to the metric, we have to impose the unimodular condition. The eqs of motion are:
• Using the Bianchi Identities and the conservation of the energy-momentum tensor, we find:
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• This differential equation can be easily integrated:
• Plugging this back in the equations of motion, one obtains
• Remarkable: on a canonical NC spacetime: the cosmological constant is an integration constant uncorrelated to parameters of the action!
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Get ready for a bit of speculation!
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• If one quantized unimodular gravity action, one finds an uncertainty relation for the cosmological constant and the volume:
• Now on a NC spacetime, the volume is “quantized”, the number of fundamental cells is expected to fluctuate
• The volume of spacetime then fluctuates with the number of cell
• In other words and one thus finds:
• Or assuming that the scale for NC is the Planck scale:
which is of the right order of magnitude!!! (critical assumption: natural value for is 0, plausible by Baum and Hawking.)
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Back to the SM of particle physics
• Let me assume that somehow gravity is taken care of at the quantum level by e.g. spacetime noncommutativity or nonperturbative effects:
• There is a good chance that Nature is indeed described by renormalizable quantum field theories.
• The remaining issue of the SM is to understand why the Higgs mechanism takes place.
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Seesaw Higgs Mechanism
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Seesaw for Higgs
• Let me consider a generic 2 Higgs doublets model
• Diagonalization of the mass matrix:
• Is there a negative root?
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• Decoupling case:
Breaks SU(2) x U(1) Decouples
Fine-tuning of the Yukawacouplings
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Degenerate case:
• Scalar potential:
• Yukawa sector:
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• Let me diagonalize the mass matrix:
• Let me assume that the action is invariant under
• This implies a symmetry for h and H.
ha ↔ hbZ2
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• In a compact notation:
• Mass spectrum
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Phenomenology
• Higgs production at LHC
• Dark matter candidate!
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A gateway to a hidden sector
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• Higgs sector is fascinating: Higgs mass term is the only super-renormalizable term in the SM: door to a hidden sector.
• New option to break the EW: e.g. hidden technicolor sector
• Connection to extra-dimension (J. van der Bij recent works)
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A simple model
• Couple a new sector in minimal way
• This operator can impact Veltman’s relation
• It improves naturalness of the SM
• Consider e.g. SM replica model
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• Different options!
• Implies interesting
new phenomenology e.g.:
and dark matter candidates
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New Guiding principles and Grand Unification
• SO(10) is viable, again due to fine tuning in Higgs sector
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Conclusions• There are two missing blocks in High Energy Physics.
• Dark energy might just be a cosmological constant which is connected to a minimal length. On a noncommutative spacetime its value is arbitrary.
• Further hand waving arguments could explain its value.
• Electroweak symmetry sector is the only SM one which has not be tested yet.
• Possible connection to hidden sectors/dark matter: LHC will produce DM in most of the scenarios.
• Were the guiding principles right?
• We will have answers soon!