Search results for "Cold"

showing 10 items of 660 documents

Mechanisms Suppressing Superheavy Element Yields in Cold Fusion Reactions.

2019

Superheavy elements are formed in fusion reactions which are hindered by fast nonequilibrium processes. To quantify these, mass-angle distributions and cross sections have been measured, at beam energies from below-barrier to 25% above, for the reactions of $^{48}\mathrm{Ca}$, $^{50}\mathrm{Ti}$, and $^{54}\mathrm{Cr}$ with $^{208}\mathrm{Pb}$. Moving from $^{48}\mathrm{Ca}$ to $^{54}\mathrm{Cr}$ leads to a drastic fall in the symmetric fission yield, which is reflected in the measured mass-angle distribution by the presence of competing fast nonequilibrium deep inelastic and quasifission processes. These are responsible for reduction of the compound nucleus formation probablity ${P}_{CN}$ …

PhysicsFissionGeneral Physics and AstronomyFission product yieldSuperheavy Elements01 natural sciences7. Clean energyCold fusionDiffusion process0103 physical sciencesNuclear fusionAtomic physics010306 general physicsEnergy (signal processing)Physical review letters
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Interpreting deviations between AR-VTG and GR

2019

The cosmic microwave background (CMB) anisotropies predicted by two cosmological models are compared, one of them is the standard model of general relativity with cold dark matter and cosmological constant, whereas the second model is based on a consistent vector-tensor theory of gravitation explaining solar system and cosmological observations. It is proved that the resulting differences — between the anisotropies of both models — are due to the so-called late integrated Sachs–Wolfe effect and, consequently, cross-correlations between maps of CMB temperatures and tracers of the dark matter distribution could be used in future to select one of the above models. The role of reionization is …

PhysicsGeneral Relativity and Quantum CosmologyCold dark matterSpace and Planetary ScienceGeneral relativityCosmic microwave backgroundAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAnisotropyMathematical PhysicsStandard ModelInternational Journal of Modern Physics D
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WMAPing the Universe: Supersymmetry, Dark Matter, Dark Energy, Proton Decay and Collider Physics

2003

In this review we discuss constraints on minimal supersymmetric models of particle physics implied by the recent astrophysical observations of WMAP. Although the prospects of detecting supersymmetry increase and 90 percent of the available MSSM parameter space can safely be reached by the sensitivity of future colliders, nevertheless we pay particular emphasis on discussing regions of the appropriate phase diagrams, which -if realized - would imply that detection of supersymmetry, at least in the context of minimal models, could be out of colliders reach. We also discuss the importance of a precise determination of the radiative corrections to the muon anomalous magnetic moment, both theore…

PhysicsHigh Energy Physics - TheoryParticle physicsAnomalous magnetic dipole momentProton decayAstrophysics (astro-ph)Dark matterFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)SupersymmetryMinimal modelsAstrophysicsCMB cold spotHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Space and Planetary ScienceDark energyMathematical Physics
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Low-Temperature Phases in Two-Orbital Hubbard Model Realized with Ultracold Atoms in Optical Lattices

2020

PhysicsHubbard modelCondensed matter physicsUltracold atomGeneral Physics and AstronomyActa Physica Polonica A
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Colliders as a simultaneous probe of supersymmetric dark matter and Terascale cosmology

2006

Terascale supersymmetry has the potential to provide a natural explanation of the dominant dark matter component of the standard lambda-CDM cosmology. However once we impose the constraints on minimal supersymmetry parameters from current particle physics data, a satisfactory dark matter abundance is no longer prima facie natural. This Neutralino Tuning Problem could be a hint of nonstandard cosmology during and/or after the Terascale era. To quantify this possibility, we introduce an alternative cosmological benchmark based upon a simple model of quintessential inflation. This benchmark has no free parameters, so for a given supersymmetry model it allows an unambiguous prediction of the da…

PhysicsInflation (cosmology)Nuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderAstrophysics (astro-ph)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaSupersymmetryAstrophysics::Cosmology and Extragalactic AstrophysicsParameter spaceAstrophysicsCMB cold spotCosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutralino
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MC calculations for the nEDM experiment systematics

2010

International audience; The nEDM experiment hosted at the Paul Scherrer Institute is the flagship project at the new ultracold neutron facility. Estimations of systematic effects for the determination of the neutron electric dipole moment play an important role in this project. Experimental studies are supported by Monte Carlo simulations using the MCUCN code. Here we briefly present first results on the experimental benchmark of the model, and on the evaluation of the storage time dependence of the centre of mass of UCN in the nEDM precession chamber. Such time dependence calculations will serve as consistency tests for future measurements involving field gradient corrections of the Ramsey…

PhysicsMC simulationsNeutron electric dipole momentField (physics)010308 nuclear & particles physicsNeutron electric dipole momentMonte Carlo methodPhysics and Astronomy(all)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNuclear physicsConsistency (statistics)Benchmark (surveying)0103 physical sciencesPrecessionUltracold neutronsNeutron010306 general physicsUltracold neutrons
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Observables sensitive to absolute neutrino masses. II

2008

In this followup to Phys. Rev. D 75, 053001 (2007) [arXiv:hep-ph/0608060] we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0nu2beta decay results in 76-Ge claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0nu2beta limits in 130-Te recently set by Cuoricino, and on prospective limits or signals from the KATRIN experiment.

PhysicsMass numberNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics (astro-ph)Cosmic background radiationFOS: Physical sciencesAstrophysicsCMB cold spotHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSDouble beta decayHigh Energy Physics::ExperimentSensitivity (control systems)Nuclear Experiment (nucl-ex)NeutrinoNeutrino oscillationNuclear ExperimentPhysical Review D
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Simulating a quantum commensurate-incommensurate phase transition using two Raman-coupled one-dimensional condensates

2020

We study a transition between a homogeneous and an inhomogeneous phase in a system of one-dimensional, Raman tunnel-coupled Bose gases. The homogeneous phase shows a flat density and phase profile, whereas the inhomogeneous ground state is characterized by periodic density ripples, and a soliton staircase in the phase difference. We show that under experimentally viable conditions the transition can be tuned by the wavevector difference $Q$ of the Raman beams and can be described by the Pokrovsky-Talapov model for the relative phase between the two condensates. Local imaging available in atom chip experiments allows to observe the soliton lattice directly, while modulation spectroscopy can …

PhysicsMesoscopic physicsPhase transitionCondensed matter physicsPhononFOS: Physical sciences02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesQuantum Gases (cond-mat.quant-gas)Ultracold atom0103 physical sciencesSoliton010306 general physics0210 nano-technologyTranslational symmetryWave functionCondensed Matter - Quantum GasesQuantum fluctuation
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First observation of trapped high-field seeking ultracold neutron spin states

2011

Ultracold neutrons were stored in a volume, using a magnetic dipole field shutter. Radial confinement was provided by material walls. Low-field seeking neutrons were axially confined above the magnetic field. High-field seeking neutrons are trapped inside the magnetic field. They can systematically shift the measured neutron lifetime to lower values in experiments with magnetic confinement. ISSN:0370-2693 ISSN:0031-9163 ISSN:1873-2445

PhysicsNeutron lifetimeNuclear and High Energy PhysicsSpin statesCondensed matter physicsUltracold neutron storage010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryMagnetic confinement fusionUltracold neutrons; Ultracold neutron storage; Neutron lifetime[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences3. Good healthMagnetic fieldShutter0103 physical sciencesUltracold neutronsNeutron010306 general physicsAxial symmetryNuclear ExperimentUltracold neutronsMagnetic dipolePhysics Letters B
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Additional results from the first dedicated search for neutron–mirror neutron oscillations

2008

International audience; The existence of a mirror world holding a copy of our ordinary particle spectrum could lead to oscillations between the neutron (n) and its mirror partner (n′). Such oscillations could manifest themselves in storage experiments with ultracold neutrons whose storage lifetime would depend on the applied magnetic field. Here, extended details and measurements from the first dedicated experimental search for nn′ oscillations published in [G. Ban, K. Bodek, M. Daum, R. Henneck, S. Heule, M. Kasprzak, N. Khomutov, K. Kirch, S. Kistryn, A. Knecht, P. Knowles, M. Kuźniak, T. Lefort, A. Mtchedlishvili, O. Naviliat-Cuncic, C. Plonka, G. Quéméner, M. Rebetez, D. Rebreyend, S. R…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsDark matter[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Mirror neutrons01 natural sciencesNeutronoscillationsMagnetic fieldNuclear physics0103 physical sciencesUltracold neutronsNeutron010306 general physicsUltracold neutronsInstrumentation
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