8,362 research outputs found
Communication through an extra dimension
If our visible universe is considered a trapped shell in a five-dimensional
hyper-universe, all matter in it may be connected by superluminal signals
traveling through the fifth dimension. Events in the shell are still causal,
however, the propagation of signals proceeds at different velocities depending
on the fifth coordinate.Comment: Latex format, 12 pages. References modifie
Decoupling Solution to SUSY Flavor Problem via Extra Dimensions
We discuss the decoupling solution to SUSY flavor problem in the fat brane
scenario. We present a simple model to yield the decoupling sfermion spectrum
in a five dimensional theory. Sfermion masses are generated by the overlap
between the wave functions of the matter fields and the chiral superfields on
the SUSY breaking brane. Two explicit examples of the spectrum are given.Comment: 8 pages, LaTe
Phenomenology of Electroweak Symmetry Breaking from Theory Space
Recently, a new class of realistic models for electroweak symmetry breaking
have been constructed, without supersymmetry. These theories have naturally
light Higgs bosons and perturbative new physics at the TeV scale. We describe
these models in detail, and show that electroweak symmetry breaking can be
triggered by a large top quark Yukawa coupling. A rich spectrum of particles is
predicted, with a pair of light Higgs doublets accompanied by new light weak
triplet and singlet scalars. The lightest of these new scalars is charged under
a geometric discrete symmetry and is therefore stable, providing a new
candidate for WIMP dark matter. At TeV energies, a plethora of new heavy
scalars, gauge bosons and fermions are revealed, with distinctive quantum
numbers and decay modes.Comment: 22 pages, latex, 6 figures. Numerical results corrected,
clarifications added, conclusions unchange
The Minimal Moose for a Little Higgs
Recently a new class of theories of electroweak symmetry breaking have been
constructed. These models, based on deconstruction and the physics of theory
space, provide the first alternative to weak-scale supersymmetry with naturally
light Higgs fields and perturbative new physics at the TeV scale. The Higgs is
light because it is a pseudo-Goldstone boson, and the quadratically divergent
contributions to the Higgs mass are cancelled by new TeV scale ``partners'' of
the {\em same} statistics. In this paper we present the minimal theory space
model of electroweak symmetry breaking, with two sites and four link fields,
and the minimal set of fermions. There are very few parameters and degrees of
freedom beyond the Standard Model. Below a TeV, we have the Standard Model with
two light Higgs doublets, and an additional complex scalar weak triplet and
singlet. At the TeV scale, the new particles that cancel the 1-loop quadratic
divergences in the Higgs mass are revealed. The entire Higgs potential needed
for electroweak symmetry breaking--the quartic couplings as well as the
familiar negative mass squared--can be generated by the top Yukawa coupling,
providing a novel link between the physics of flavor and electroweak symmetry
breaking.Comment: 15 pages. References added. Included clarifying comments on the
origin of quartic couplings, and on power-counting. More elegant model for
generating Higgs potential from top Yukawa coupling presente
Ghost Cosmology: Exact Solutions, Transitions Between Standard Cosmologies and Ghost Dark Energy/Matter Evolution
The recently proposed infrared modification of gravity through the
introduction of a ghost scalar field results in a number of interesting
cosmological and phenomenological implications. In this paper, we derive the
exact cosmological solutions for a number of scenarios where at late stages,
the ghost behaves like dark matter, or dark energy. The full solutions give
valuable information about the non-linear regime beyond the asymptotic first
order analysis presented in the literature. The generic feature is that these
ghost cosmologies give rise to smooth transitions between radiation dominated
phases (or more general power-law expansions) at early epochs and ghost dark
matter resp. ghost dark energy dominated late epochs. The current age of our
universe places us right at the non-linear transition phase. By studying the
evolution backwards in time, we find that the dominance of the ghost over
ordinary baryonic matter and radiative contributions persists back to the
earliest times such that the Friedmann-Robertson-Walker geometry is dictated to
a good approximation by the ghost alone. We also find that the Jeans
instability occurs in the ghost dark energy scenario at late times, while it is
absent in the ghost dark matter scenario.Comment: 31 pages, 9 figures; added references, clarified a few minor point
Single production of new gauge bosons from the littlest Higgs model at the energy colliders
In the context of the littlest Higgs(LH) model, we study single production of
the new gauge bosons , and via
collisions and discuss the possibility of detecting these new particles in the
energy collider(). We find that these new particles can
not be detected via the signal in all of the parameter space
preferred by the electroweak precision data. However, the heavy gauge bosons
and may be observed via the decay channel in wide range of the parameter space.Comment: references added, typos corrected. To be published in Phys. Rev.
The Momentum Amplituhedron
In this paper we define a new object, the momentum amplituhedron, which is the long sought-after positive geometry for tree-level scattering amplitudes in N = 4 super Yang-Mills theory in spinor helicity space. Inspired by the construction of the ordinary amplituhedron, we introduce bosonized spinor helicity variables to represent our external kinematical data, and restrict them to a particular positive region. The momentum amplituhedron M n,k is then the image of the positive Grassmannian via a map determined by such kinematics. The scattering amplitudes are extracted from the canonical form with logarithmic singularities on the boundaries of this geometry.Peer reviewedFinal Published versio
A numerical study of the temperature field in a cooled radial turbine rotor
The three dimensional temperature distribution in the cooled rotor of a radial inflow turbine is determined numerically using the finite element method. Through this approach, the complicated geometries of the hot rotor and coolant passage surfaces are handled easily, and the temperatures are determined without loss of accuracy at these convective boundaries. Different cooling techniques with given coolant to primary flow ratios are investigated, and the corresponding rotor temperature fields are presented for comparison
The Long Range Gravitational Potential Energy Between Strings
We calculate the gravitational potential energy between infinitely long
parallel strings with tensions \tau_1 and \tau_2. Classically, it vanishes, but
at one loop, we find that the long range gravitational potential energy per
unit length is U/L = 24G_N^2\tau_1\tau_2/(5 \pi a^2) + ..., where a is the
separation between the strings, G_N is Newton's constant, and we set \hbar = c
=1. The ellipses represent terms suppressed by more powers of G_N \tau_i.
Typically, massless bulk fields give rise at one loop to a long range potential
between p-branes in space-times of dimension p+2+1. The contribution to this
potential from bulk scalars is computed for arbitrary p (strings correspond to
p=1) and in the case of three-branes its possible relevance for cosmological
quintessence is commented on.Comment: 10 pages, 6 figure
Viable Ultraviolet-Insensitive Supersymmetry Breaking
It is known that one can add D-term contributions for U(1)_Y and U(1)_{B-L}
to the anomaly-mediated supersymmetry breaking to make the superparticle
spectrum phenomenologically viable. We point out that this can be done without
spoiling its important virtue, namely the ultraviolet insensitivity. This
framework can be derived from supersymmetry breaking and U(1)_{B-L} breaking on
hidden brane(s).Comment: 19 pages, Latex, small clarifications adde
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