Search results for " Bounds"

showing 10 items of 291 documents

Hefty MSSM-like light Higgs in extended gauge models

2011

It is well known that in the MSSM the lightest neutral Higgs h^0 must be, at the tree level, lighter than the Z boson and that the loop corrections shift this stringent upper bound up to about 130 GeV. Extending the MSSM gauge group in a suitable way, the new Higgs sector dynamics can push the tree-level mass of h^0 well above the tree-level MSSM limit if it couples to the new gauge sector. This effect is further pronounced at the loop level and h^0 masses in the 140 GeV ballpark can be reached easily. We exemplify this for a sample setting with a low-scale U(1)_R x U(1)_B-L gauge symmetry in which neutrino masses can be implemented via the inverse seesaw mechanism.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaGauge (firearms)01 natural sciencesUpper and lower boundsHiggs sectorHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Gauge group0103 physical sciencesHiggs bosonHigh Energy Physics::ExperimentNeutrino010306 general physicsGauge symmetry
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Current cosmological bounds on neutrino masses and relativistic relics

2004

We combine the most recent observations of large-scale structure (2dF and SDSS galaxy surveys) and cosmic microwave anisotropies (WMAP and ACBAR) to put constraints on flat cosmological models where the number of massive neutrinos and of massless relativistic relics are both left arbitrary. We discuss the impact of each dataset and of various priors on our bounds. For the standard case of three thermalized neutrinos, we find an upper bound on the total neutrino mass sum m_nu < 1.0 (resp. 0.6) eV (at 2sigma), using only CMB and LSS data (resp. including priors from supernovae data and the HST Key Project), a bound that is quite insensitive to the splitting of the total mass between the th…

PhysicsNuclear and High Energy PhysicsParticle physicsCosmic microwave backgroundDark matterAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsUpper and lower boundsCMB cold spotMassless particleHigh Energy Physics - PhenomenologySupernovaHigh Energy Physics - Phenomenology (hep-ph)Observational cosmologyNeutrino
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Predicting Neutrinoless Double Beta Decay

2005

We give predictions for the neutrinoless double beta decay rate in a simple variant of the A_4 family symmetry model. We show that there is a lower bound for the neutrinoless double beta decay amplitude even in the case of normal hierarchical neutrino masses, corresponding to an effective mass parameter |m_{ee}| >= 0.17 \sqrt{\Delta m^2_{ATM}}. This result holds both for the CP conserving and CP violating cases. In the latter case we show explicitly that the lower bound on |m_{ee}| is sensitive to the value of the Majorana phase. We conclude therefore that in our scheme, neutrinoless double beta decay may be accessible to the next generation of high sensitivity experiments.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaUpper and lower boundsMAJORANAHigh Energy Physics - PhenomenologyEffective mass (solid-state physics)AmplitudeHigh Energy Physics - Phenomenology (hep-ph)Double beta decayCP violationHigh Energy Physics::ExperimentNeutrinoSimple variant
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Double beta decay versus cosmology: Majorana CP phases and nuclear matrix elements

2004

We discuss the relation between the absolute neutrino mass scale, the effective mass measured in neutrinoless double beta decay, and the Majorana CP phases. Emphasis is placed on estimating the upper bound on the nuclear matrix element entering calculations of the double beta decay half life. Consequently, one of the Majorana CP phases can be constrained when combining the claimed evidence for neutrinoless double beta decay with the neutrino mass bound from cosmology.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesUpper and lower boundsNuclear physicsMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Effective mass (solid-state physics)Double beta decayCP violationHigh Energy Physics::ExperimentNeutrinoRandom phase approximationNeutrino oscillation
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Absolute neutrino mass scale from flavor symmetries

2013

Abstract The 2012 has been an important year for neutrino physics, current data are reviewed and compared with 2011 global fit. Models based on discrete flavor symmetries predict neutrino mass mass sum-rule (MSR), which is useful to reduce the number of independent model parameters. We found that only four classes of MSR are possible. Such neutrino MSRs constrain the absolute neutrino mass scale. We study the implications of these mass relations for the lightest neutrino mass and for the lower bound of the effective mass m e e of the neutrinoless double beta decay.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyUpper and lower boundsAtomic and Molecular Physics and OpticsNuclear physicsEffective mass (solid-state physics)Double beta decayHomogeneous spaceMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationFlavorNuclear Physics B - Proceedings Supplements
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Neutral Higgs sector of the MSSM without R-p

1999

We analyse the neutral scalar sector of the MSSM without R-parity. Our analysis is performed for a one-generation model in terms of ``basis-independent'' parameters, and includes one-loop corrections due to large yukawa couplings. We concentrate on the consequences of large $R_p$ violating masses in the soft sector, which mix the Higgses with the sleptons, because these are only constrained by their one-loop contributions to neutrino masses. We focus on the effect of $R_p$-violation on the Higgs mass and branching ratios. We find that the experimental lower bound on the lightest CP-even Higgs in this model can be lower than in the MSSM.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciencesFísicaUpper and lower boundsHiggs sectorHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Higgs bosonHigh Energy Physics::ExperimentNeutrinoParticle Physics - Phenomenology
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Spontaneous CP violation and the B0 system

1998

We investigate effects of spontaneous breakdown of CP in $B^0_{d,s}-\overline{B^0}_{d,s}$ systems in left-right symmetric models. Assuming that the left-right contribution to the $B^0-\overline{B^0}$ matrix element $M_{12}$ can be at most equal to the standard model one we obtain a new lower bound, $M_H\gsim 12$ TeV, on the flavour changing Higgs boson mass. Most importantly, the convention independent parameter $Re(\overline{\epsilon}_B),$ which measures the amount of $\Delta B=2$ CP violation, can be enhanced by a factor of four or more for $B^0_d$ and almost by two orders of magnitude for $B^0_s$ systems when compared with the Standard Model predictions. Therefore, interesting possibilit…

PhysicsNuclear and High Energy PhysicsParticle physicsIndependent parameterHiggs bosonFísicaCP violationMatrix elementUpper and lower boundsOrder of magnitudeStandard ModelNuclear Physics B
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Cornering Colored Coannihilation

2018

In thermal dark matter models, allowing the dark matter candidate to coannihilate with another particle can considerably loosen the relic density constraints on the dark matter mass. In particular, introducing a single strongly interacting coannihilation partner in a dark matter model can bring the upper bound on the dark sector energy scale from a few TeV up to about 10 TeV. While these energies are outside the LHC reach, a large part of the parameter space for such coannihilating models can be explored by future hadron colliders. In this context, it is essential to determine whether the current bounds on dark matter simplified models also hold in non-minimal scenarios. In this paper, we s…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsDark matterHadronFOS: Physical sciencesContext (language use)Minimal modelsAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesUpper and lower boundslaw.inventionHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)law0103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsColliderPhenomenological Models
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Search for the rare decayBs0→ϕμ+μ−with the D0 detector

2006

We present a search for the flavor-changing neutral current decay B-s(0)->phi mu(+)mu(-) using about 0.45 fb(-1) of data collected in p (p) over bar collisions at root s=1.96 TeV with the D0 detector at the Fermilab Tevatron Collider. We find an upper limit on the branching ratio of this decay normalized to B-s(0)-> J/psi phi of B(B-s(0)->phi mu(+)mu(-))/B(B-s(0)-> J/psi phi) J/psi phi, the limit corresponds to B(B-s(0)->phi mu(+)mu(-))< 4.1x10(-6) at the 95% C.L., the most stringent upper bound to date.

PhysicsNuclear and High Energy PhysicsParticle physicsNeutral current010308 nuclear & particles physicsBranching fractionDetectorTevatron01 natural sciencesUpper and lower boundslaw.inventionlaw0103 physical sciencesHigh Energy Physics::ExperimentFermilab010306 general physicsColliderBar (unit)Physical Review D
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Pionic decay of Lambda Hypernuclei in a Continuum Shell Model

2002

We evaluate pionic decay widths of Lambda hypernuclei using a shell model for, both the nuclear bound and the continuum nucleon wave functions in the final state, and distorted waves for the outgoing pion. An excellent agreement with the recent KEK measurement of $\pi^-$-decay widths of $^{12}_\Lambda$C and $^{28}_\Lambda$Si is found. Besides, results for $^{56}_\Lambda$Fe are consistent with the existing upper bound.

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheorySHELL modelNuclear TheoryFísicaFOS: Physical sciencesState (functional analysis)LambdaUpper and lower boundsNuclear Theory (nucl-th)PionHigh Energy Physics::ExperimentContinuum (set theory)Atomic physicsNucleonWave functionNuclear Experiment
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