1,476 research outputs found
Nuclear shell evolution and in-medium NN interaction
We report on a quantitative study of the evolution of the nuclear shell structure, in particular, effective single-particle energies (ESPEs), based on the spin-tensor decomposition of an effective two-body shell-model interaction. While the global trend of the ESPEs is mainly due to the central term of the effective interaction, variations of shell gaps invoke various components of the in-medium NN force. From a detailed analysis of a well-fitted realistic interaction in the sdpf shell-model space, two most important contributions for the evolution of the N = 20 and N = 28 shell gaps are confirmed to be the central term and the tensor term. The role of the latter is dominant to explain the energy shift of spin-orbit partners. Spin-tensor analysis of microscopic effective interactions in sd, pf, and gds shell-model spaces, contrasted with that of the phenomenologically adjusted ones, shows no evidence of amplification of the tensor component contribution; however, it points toward the neglect of three-body forces in the present microscopic interactions
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Direct Imaging At 12 Microns Of The Star-Forming Region W51 IRS-2
Astronom
The Hierarchy Problem and the Top Yukawa: An Alternative to Top Partner Solutions
We discuss the role of the top-quark Yukawa coupling concerning thehierarchy problem and construct an alternative scheme to the conventionalsolutions with top partners. In traditional models, like SUSY or compositeHiggs, top partners cancel the top loop contribution to the Higgs quadraticterm. The lack of evidence for such colored partners however drives thesemodels into more and more fine-tuned regions. Here, an alternative means tomitigate the top loop, allowing for natural electroweak symmetry breaking, ispresented. Emphasizing that we have not measured the top-Higgs interactions athigh scales yet, we envisage scenarios where this interaction is onlyapproaching its sizable strength in the infra-red, but gets strongly suppressedat high scales. We first discuss possible effects via a modification of therunning of the top Yukawa coupling. Then, we turn to models where the topYukawa is generated at one-loop level. Originated from a dimension-sixoperator, it drops when crossing the mass threshold of new degrees of freedom.In either case, the top partners are replaced by some new top-philic particleswith strong interaction. Thus, a very different phenomenology, such as largetop mass running and signals in four top final states, is introduced, whichwill be discussed in detail. With the assistance of this mechanism, thesolution to the hierarchy problem can be pushed to a (well-defined) higherscale, and a final test of naturalness might be deferred to a 100 TeV Collider,like the FCC.<br
The Hierarchy Problem and the Top Yukawa: An Alternative to Top Partner Solutions
We discuss the role of the top-quark Yukawa coupling concerning thehierarchy problem and construct an alternative scheme to the conventionalsolutions with top partners. In traditional models, like SUSY or compositeHiggs, top partners cancel the top loop contribution to the Higgs quadraticterm. The lack of evidence for such colored partners however drives thesemodels into more and more fine-tuned regions. Here, an alternative means tomitigate the top loop, allowing for natural electroweak symmetry breaking, ispresented. Emphasizing that we have not measured the top-Higgs interactions athigh scales yet, we envisage scenarios where this interaction is onlyapproaching its sizable strength in the infra-red, but gets strongly suppressedat high scales. We first discuss possible effects via a modification of therunning of the top Yukawa coupling. Then, we turn to models where the topYukawa is generated at one-loop level. Originated from a dimension-sixoperator, it drops when crossing the mass threshold of new degrees of freedom.In either case, the top partners are replaced by some new top-philic particleswith strong interaction. Thus, a very different phenomenology, such as largetop mass running and signals in four top final states, is introduced, whichwill be discussed in detail. With the assistance of this mechanism, thesolution to the hierarchy problem can be pushed to a (well-defined) higherscale, and a final test of naturalness might be deferred to a 100 TeV Collider,like the FCC.<br
SU(6) Gauge-Higgs Grand Unification: Minimal Viable Models and Flavor
Gauge-Higgs grand unification theories are models of gauge-Higgs unification that extend the electroweak group into a simple group that includes the color symmetry. The minimal option is a gauge-Higgs grand unification based on the SU(6) gauge group, mirroring SU(5) grand unification in 4D while providing a solution to the hierarchy problem. We explore different minimal and realistic novel incarnations of SU(6) gauge-Higgs grand unification. We submit the setup to the various flavor hierarchies observed in nature and, utilizing the power of the fifth dimension, identify an embedding that provides a compelling model of quarks and leptons that naturally explains the mass hierarchies and the CKM/PMNS structure. We perform a detailed study of quark - and lepton - flavor constraints (which are intimately related due to the GUT nature) together with an analysis of the Higgs potential which arises at the loop level. Electroweak precision constraints on the model are discussed and the rich scalar sector is analyzed. Future flavor constraints from upcoming experiments will provide a stringent test for this class of models, while a scalar singlet and leptoquark provide unique targets for current and future collider experiments to probe this solution to various open questions in nature
Unification of Gauge Symmetries... including their breaking
In this talk, we present a minimal viable scenario that unifies the gaugesymmetries of the Standard Model (SM) and their breaking sector. OurGauge-Higgs Grand Unification setup employs 5D warped space with a bulkgauge field that includes both a grand unified theory (GUT) and a Higgssector as a scalar component of the 5D vector field, solving the hierarchyproblem. By appropriately breaking the gauge symmetry on the boundaries of theextra dimension the issue of light exotic new states, appearing generically insuch models, is eliminated and the SM fermion spectrum is naturally reproduced.The Higgs potential is computed at one-loop, finding straightforward solutionswith a realistic GeV. The problem of proton decay is addressed byshowing that baryon number is a hidden symmetry of the model. The presence of ascalar leptoquark and a scalar singlet is highlighted, which might play a rolein solving further problems of the SM, allowing for example for electroweakbaryogenesis. Finally, the and gauge bosons from GUTs are foundat collider accessible masses, opening a window to the unification structure atlow energies.<br
Large Area Mapping at 850 Microns. V. Analysis of the Clump Distribution in the Orion A South Molecular Cloud
We present results from a 2300 arcmin^2 survey of the Orion A molecular cloud
at 450 and 850 micron using the Submillimetre Common-User Bolometer Array
(SCUBA) on the James Clerk Maxwell Telescope. The region mapped lies directly
south of the OMC1 cloud core and includes OMC4, OMC5, HH1/2, HH34, and L1641N.
We identify 71 independent clumps in the 850 micron map and compute size, flux,
and degree of central concentration in each. Comparison with isothermal,
pressure-confined, self-gravitating Bonnor-Ebert spheres implies that the
clumps have internal temperatures T_d ~ 22 +/- K and surface pressures log
(k^-1 P cm^-3 K) = 6.0 +/- 0.2. The clump masses span the range 0.3 - 22 Msun
assuming a dust temperature T_d ~ 20 K and a dust emissivity kappa_850 = 0.02
cm^2 g^-1. The distribution of clump masses is well characterized by a
power-law N(M) propto M^-alpha with alpha = 2.0 +/- 0.5 for M > 3.0 Msun,
indicating a clump mass function steeper than the stellar Initial Mass
Function. Significant incompleteness makes determination of the slope at lower
masses difficult. A comparison of the submillimeter emission map with an H_2
2.122 micron survey of the same region is performed. Several new Class 0
sources are revealed and a correlation is found between both the column density
and degree of concentration of the submillimeter sources and the likelihood of
coincident H_2 shock emission.Comment: 44 pages, 17 figures, accepted by Ap
An S-shaped outflow from IRAS 03256+3055 in NGC 1333
The IRAS source 03256+3055 in the NGC 1333 star forming region is associated
with extended sub-millimeter emission of complex morphology, showing multiple
clumps. One of these is found to coincide with the driving source of a bipolar
jet of S-shaped morphology seen in the emission lines of H_alpha and [SII] as
well as in the H2 emission lines in the K-band. Detailed images of the driving
source at the wavelengths of H_alpha and [SII] and in the I, J, H, and K bands
as well as a K-band spectrum and polarimetry are discussed. The near-infrared
morphology is characterized by a combination of line emission from the jet and
scattered light from a source with a steep continuum spectrum. The morphology
and proper motion of the jet are discussed in the context of a binary system
with a precessing disk. We conclude that the molecular core associated with
IRAS 03256+3055 consists of several clumps, only one of which shows evidence of
recent star formation at optical and near-infrared wavelengths.We also briefly
discuss a second, newly found near-infrared source associated with a compact
sub-millimeter continuum source near IRAS 03256+3055, and conclude that this
source may be physically unrelated the cluster of molecular clumps.Comment: 25 pages, including 5 figures. Accepted for publication in The
Astronomical Journa
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