19,873 research outputs found
Singlet Model Interference Effects with High Scale UV Physics
One of the simplest extensions of the Standard Model (SM) is the addition of
a scalar gauge singlet, S. If S is not forbidden by a symmetry from mixing with
the Standard Model Higgs boson, the mixing will generate non-SM rates for Higgs
production and decays. In general, there could also be unknown high energy
physics that generates additional effective low energy interactions. We show
that interference effects between the scalar resonance of the singlet model and
the effective field theory (EFT) operators can have significant effects in the
Higgs sector. We examine a non- symmetric scalar singlet model and
demonstrate that a fit to the 125 GeV Higgs boson couplings and to limits on
high mass resonances, S, exhibit an interesting structure and possible large
cancellations of effects between the resonance contribution and the new EFT
interactions, that invalidate conclusions based on the renormalizable singlet
model alone.Comment: 18 pages, 7 figures; revised to emphasize the points of general
interest for heavy resonance searches at the LH
Neptune's wild days: constraints from the eccentricity distribution of the classical Kuiper Belt
Neptune's dynamical history shaped the current orbits of Kuiper belt objects
(KBOs), leaving clues to the planet's orbital evolution. In the "classical"
region, a population of dynamically "hot" high-inclination KBOs overlies a flat
"cold" population with distinct physical properties. Simulations of
qualitatively different histories for Neptune -including smooth migration on a
circular orbit or scattering by other planets to a high eccentricity - have not
simultaneously produced both populations. We explore a general Kuiper belt
assembly model that forms hot classical KBOs interior to Neptune and delivers
them to the classical region, where the cold population forms in situ. First,
we present evidence that the cold population is confined to eccentricities well
below the limit dictated by long-term survival. Therefore Neptune must deliver
hot KBOs into the long-term survival region without excessively exciting the
eccentricities of the cold population. Imposing this constraint, we explore the
parameter space of Neptune's eccentricity and eccentricity damping, migration,
and apsidal precession. We rule out much of parameter space, except where
Neptune is scattered to a moderately eccentric orbit (e > 0.15) and
subsequently migrates a distance Delta aN=1-6 AU. Neptune's moderate
eccentricity must either damp quickly or be accompanied by fast apsidal
precession. We find that Neptune's high eccentricity alone does not generate a
chaotic sea in the classical region. Chaos can result from Neptune's
interactions with Uranus, exciting the cold KBOs and placing additional
constraints. Finally, we discuss how to interpret our constraints in the
context of the full, complex dynamical history of the solar system.Comment: Corrected typos and made wording changes. Corrected Fig. 8 (row 2)
and Fig. 17. Reduced loading time of Fig. 1
Top Partners and Higgs Boson Production
The Higgs boson is produced at the LHC through gluon fusion at roughly the
Standard Model rate. New colored fermions, which can contribute to
, must have vector-like interactions in order not to be in
conflict with the experimentally measured rate. We examine the size of the
corrections to single and double Higgs production from heavy vector-like
fermions in singlets and doublets and search for regions of parameter
space where double Higgs production is enhanced relative to the Standard Model
prediction. We compare production rates and distributions for double Higgs
production from gluon fusion using an exact calculation, the low energy theorem
(LET), where the top quark and the heavy vector-like fermions are taken to be
infinitely massive, and an effective theory (EFT) where top mass effects are
included exactly and the effects of the heavy fermions are included to . Unlike the LET, the EFT gives an extremely accurate description
of the kinematic distributions for double Higgs production.Comment: 37 pages, 11 figures. Minor changes to Figs. 8-1
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