Search results for "ddc:"

showing 10 items of 3080 documents

Horizons: Nuclear Astrophysics in the 2020s and Beyond

2022

Nuclear astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the chemical elements. This white paper summarizes progress and status of the field, the new open questions that have emerged, and the tremendous scientific opportunities that have opened up with major advances in capabilities across an ever growing number of disciplines and subfields that need to be integrated.We take a holistic view of the field discussing the unique challenges and opportunities in nuclear astrophysics in regards to science, diversity, education, and the interdisciplinarity and breadth of the field…

High Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsNuclear TheoryComputingMethodologies_SIMULATIONANDMODELINGastrofysiikkaStarke Wechselwirkung und exotische Kerne – Abteilung BlaumWhite PaperFOS: Physical sciencesReviewtutkimustoimintatutkimuskohteet530Nuclear Theory (nucl-th)Astrophysics - Solar and Stellar AstrophysicsNuclear astrophysicsddc:530Nuclear Experiment (nucl-ex)ydinfysiikkaAstrophysics - High Energy Astrophysical PhenomenaNuclear ExperimenttiedeyhteisötSolar and Stellar Astrophysics (astro-ph.SR)
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Measurement of the cosmic ray energy spectrum with IceTop-73

2013

Physical review / D 88(4), 042004 (2013). doi:10.1103/PhysRevD.88.042004

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsFOS: Physical sciencesAstronomyCosmic rayddc:500.2Astrophysics53001 natural sciencesPower lawICECUBEIceCubeIceCube Neutrino ObservatoryAir showerPhysics and AstronomyObservatory0103 physical sciencesEnergy spectrumARRAYddc:530Astrophysics - High Energy Astrophysical Phenomena010306 general physicsphysics
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Modified majoron model for cosmological anomalies

2020

The vacuum expectation value $v_s$ of a Higgs triplet field $\Delta$ carrying two units of lepton number $L$ induces neutrino masses $\propto v_s$. The neutral component of $\Delta$ gives rise to two Higgs particles, a pseudoscalar $A$ and a scalar $S$. The most general renormalizable Higgs potential $V$ for $\Delta $ and the Standard-Model Higgs doublet $\Phi$ does not permit the possibility that the mass of either $A$ or $S$ is small, of order $v_s$, while the other mass is heavy enough to forbid the decay $Z\to A S$ to comply with LEP 1 data. We present a model with additional dimension-6 terms in $V$, in which this feature is absent and either $A$ or $S$ can be chosen light. Subsequentl…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesOrder (ring theory)01 natural sciencesLepton numberPseudoscalarHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHiggs bosonddc:530High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsVacuum expectation valueMajoronBosonPhysical Review D
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Search for invisible decays of the Λ baryon

2022

Physical review / D 105(7), L071101 (2022). doi:10.1103/PhysRevD.105.L071101

High Energy Physics - Experiment (hep-ex)High Energy Physics::PhenomenologyFOS: Physical sciencesddc:530High Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics530
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Fully nonperturbative charm-quark tuning using machine learning

2022

We present a relativistic heavy-quark action tuning for the charm sector on ensembles generated by the CLS consortium. We tune a particular 5-parameter action in an entirely non-perturbative and -- up to the chosen experimental input -- model-independent way using machine learning and the continuum experimental charmonium ground-state masses with various quantum numbers. In the end we are reasonably successful; obtaining a set of simulation parameters that we then verify produces the expected spectrum. In the future, we will use this action for finite-volume calculations of hadron-hadron scattering.

High Energy Physics - Lattice530 PhysicsHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyFOS: Physical sciencesddc:530High Energy Physics::Experiment530 Physik530
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Spectral signatures of axionlike dark matter

2022

We derive spectral line shapes of the expected signal for a haloscope experiment searching for axionlike dark matter. The knowledge of these line shapes is needed to optimize an experimental design and data analysis procedure. We extend the previously known results for the axion-photon and axion-gluon couplings to the case of gradient (axion-fermion) coupling. A unique feature of the gradient interaction is its dependence not only on magnitudes but also on directions of velocities of galactic halo particles, which leads to the directional sensitivity of the corresponding haloscope. We also discuss the daily and annual modulations of the gradient signal caused by the Earth's rotational and o…

High Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)FOS: Physical sciencesddc:530530Astrophysics - Cosmology and Nongalactic AstrophysicsHigh Energy Physics - ExperimentPhysics - Atomic PhysicsPhysical Review
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Isovector Axial Form Factor of the Nucleon from Lattice QCD

2022

The isovector axial form factor of the nucleon plays a key role in interpreting data from long-baseline neutrino oscillation experiments. We present a lattice QCD calculation of this form factor, introducing a new method to directly extract its z-expansion from lattice correlators. Our final parameterization of the form factor, which extends up to spacelike virtualities of 0.7 GeV^2 with fully quantified uncertainties, agrees with previous lattice calculations but is significantly less steep than neutrino-deuterium scattering data suggests.

High Energy Physics - PhenomenologyHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)530 PhysicsHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesddc:530530 Physik530
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Pseudovector and pseudoscalar spin-dependent interactions in atoms

2019

Hitherto unknown elementary particles can be searched for with atomic spectroscopy. We conduct such a search using a potential that results from the longitudinal polarization of a pseudovector particle. We show that such a potential, inversely proportional to the boson's mass squared, $V \propto 1/M^2$, can stay finite at $M \to 0$ if the theory is renormalizable. We also look for a pseudoscalar boson, which induces a contact spin-dependent potential that does not contribute to new forces searched for in experiments with macroscopic objects, but may be seen in atomic spectroscopy. We extract limits on the interaction constants of these potentials from the experimental spectra of antiprotoni…

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Atomic Physics (physics.atom-ph)FOS: Physical sciencesddc:530Physics::Atomic PhysicsPhysics - Atomic Physics
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Lattice calculation of the pion transition form factor with $N_f=2+1$ Wilson quarks

2019

Physical review / D D 100(3), 034520 (2019). doi:10.1103/PhysRevD.100.034520

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesddc:530High Energy Physics::Experiment530
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Impact of nuclear matrix element calculations for current and future neutrinoless double beta decay searches

2023

Nuclear matrix elements (NME) are a crucial input for the interpretation of neutrinoless double beta decay data. We consider a representative set of recent NME calculations from different methods and investigate the impact on the present bound on the effective Majorana mass $m_{\beta\beta}$ by performing a combined analysis of the available data as well as on the sensitivity reach of future projects. A crucial role is played by the recently discovered short-range contribution to the NME, induced by light Majorana neutrino masses. Depending on the NME model and the relative sign of the long- and short-range contributions, the current $3\sigma$ bound can change between $m_{\beta\beta} < 40$ m…

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)PhysicsFOS: Physical sciencesddc:530Journal of High Energy Physics
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