3,694 research outputs found
Right-Handed Neutrinos as the Origin of the Electroweak Scale
The insular nature of the Standard Model may be explained if the Higgs mass
parameter is only sensitive to quantum corrections from physical states.
Starting from a scale-free electroweak sector at tree-level, we postulate that
quantum effects of heavy right-handed neutrinos induce a mass term for a scalar
weak doublet that contains the dark matter particle. In turn, below the scale
of heavy neutrinos, the dark matter sector sets the scale of the Higgs
potential. We show that this framework can lead to a Higgs mass that respects
physical naturalness, while also providing a viable scalar dark matter
candidate, realistic light neutrino masses, and the baryon asymmetry of the
Universe via leptogenesis. The proposed scenario can remain perturbative and
stable up to the Planck scale, thereby accommodating simple extensions to
include a high scale (2\times 10^{16} GeV) inflationary sector, implied by
recent measurements. In that case, our model typically predicts that the dark
matter scalar is close to 1 TeV in mass and could be accessible in near future
direct detection experiments.Comment: Revtex4, 10 pages, 6 figures. An appendix on a classically scale
invariant scenario for right-handed neutrino masses, as well as new
references added. Version accepted for publication in PR
Dark Matter from Hidden Forces
We examine the possibility that dark matter may be the manifestation of dark
forces of a hidden sector, i.e. "Dark Force = Dark Matter." As an illustrative
and minimal example we consider the hidden SU(2)_h x U(1)_h gauge group. The
hidden dynamics is indirectly coupled to the Standard Model (SM) through
kinetic mixing of U(1)_h with the U(1)_Y of hypercharge. We assume a hidden
symmetry breaking pattern analogous to that of the SM electroweak symmetry,
augmented with an extra scalar that allows both the "hidden Z boson" Z_h and
the "hidden photon" \gamma_h to be massive. The "hidden W" bosons W_h are dark
matter in this scenario. This setup can readily accommodate a potential direct
detection signal for dark matter at ~10 GeV from CDMSII-Si data. For some
choices of parameters, the model can lead to signals both in "dark matter beam"
experiments, from Z_h\to W_h W_h, as well as in experiments that look for
visible signals of dark photons, mediated by \gamma_h. Other possible
phenomenological consequences are also briefly discussed.Comment: 11 pages, 4 figures; References and additional comments added.
Results unchange
Invariant random subgroups of semidirect products
We study invariant random subgroups (IRSs) of semidirect products . In particular, we characterize all IRSs of parabolic subgroups
of , and show that all ergodic IRSs of are either of the form for some IRS of , or are induced from IRSs of
, where is a
lattice.Comment: 16 page
Electroweak Phase Transition, Higgs Diphoton Rate, and New Heavy Fermions
We show that weak scale vector-like fermions with order one couplings to the
Higgs can lead to a novel mechanism for a strongly first-order electroweak
phase transition (EWPhT), through their tendency to drive the Higgs quartic
coupling negative. These same fermions could also enhance the loop-induced
branching fraction of the Higgs into two photons, as suggested by the recent
discovery of a ~125 GeV Higgs-like state at the CERN Large Hadron Collider
(LHC). Our results suggest that measurements of the diphoton decay rate of the
Higgs and its self coupling, at the LHC or perhaps at a future lepton collider,
could probe the EWPhT in the early Universe, with significant implications for
the viability of electroweak baryogenesis scenarios.Comment: 6 pages, 1 figure. Revised version shows that the original
conclusions hold in a distinct region of parameter space. New discussion on
collider probes adde
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