0000000000008678

AUTHOR

Benjamin Roberts

showing 8 related works from this author

Limiting P-odd interactions of cosmic fields with electrons, protons and neutrons

2014

We propose methods for extracting limits on the strength of P-odd interactions of pseudoscalar and pseudovector cosmic fields with electrons, protons and neutrons. Candidates for such fields are dark matter (including axions) and dark energy, as well as several more exotic sources described by standard-model extensions. Calculations of parity nonconserving amplitudes and atomic electric dipole moments induced by these fields are performed for H, Li, Na, K, Rb, Cs, Ba+, Tl, Dy, Fr, and Ra+. From these calculations and existing measurements in Dy, Cs and Tl, we constrain the interaction strengths of the parity-violating static pseudovector cosmic field to be 7*10^(-15) GeV with an electron, a…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)ProtonNuclear TheoryAtomic Physics (physics.atom-ph)Dark matterNuclear TheoryGeneral Physics and AstronomyFOS: Physical sciencesElectronSpace Physics (physics.space-ph)Physics - Atomic PhysicsNuclear physicsPseudoscalarNuclear Theory (nucl-th)DipoleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics - Space PhysicsNeutronPseudovectorAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark matter scattering on electrons: Accurate calculations of atomic excitations and implications for the DAMA signal

2016

We revisit the WIMP-type dark matter scattering on electrons that results in atomic ionization and can manifest itself in a variety of existing direct-detection experiments. Unlike the WIMP-nucleon scattering, where current experiments probe typical interaction strengths much smaller than the Fermi constant, the scattering on electrons requires a much stronger interaction to be detectable, which in turn requires new light force carriers. We account for such new forces explicitly, by introducing a mediator particle with scalar or vector couplings to dark matter and to electrons. We then perform state-of-the-art numerical calculations of atomic ionization relevant to the existing experiments.…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)010308 nuclear & particles physicsScatteringPhysics beyond the Standard ModelDark matterScalar (mathematics)FOS: Physical sciencesElectron01 natural sciencesHigh Energy Physics - ExperimentPhysics - Atomic PhysicsComputational physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Ionization0103 physical sciencesAtomic physics010306 general physicsRelativistic quantum chemistryAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space TelescopePhysical Review D
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Comment on "Axion induced oscillating electric dipole moments"

2017

In the recent work [Phys. Rev. D 91, 111702(R) (2015)], C. Hill concludes that the axion electromagnetic anomaly induces an oscillating electron electric dipole moment of frequency $m_a$ and strength $\sim 10^{-32}~e$ cm, in the limit $v/c \to 0$ for the axion field. Here, we demonstrate that a proper treatment of this problem in the lowest order yields $\textit{no}$ electric dipole moment of the electron in the same limit. Instead, oscillating electric dipole moments of atoms and molecules are produced by different mechanisms.

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)Atomic Physics (physics.atom-ph)010308 nuclear & particles physicsFOS: Physical sciencesOrder (ring theory)Electron01 natural sciencesElectron electric dipole momentPhysics - Atomic PhysicsDipoleElectric dipole momentHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum mechanics0103 physical sciencesAnomaly (physics)Atomic physics010306 general physicsAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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Electron-interacting dark matter: Implications from DAMA/LIBRA-phase2 and prospects for liquid xenon detectors and NaI detectors

2019

We investigate the possibility for the direct detection of low-mass (GeV scale) weakly interacting massive particles (WIMP) dark matter in scintillation experiments. Such WIMPs are typically too light to leave appreciable nuclear recoils but may be detected via their scattering off atomic electrons. In particular, the DAMA Collaboration [R. Bernabei et al., Nucl. Phys. At. Energy 19, 307 (2018)] has recently presented strong evidence of an annual modulation in the scintillation rate observed at energies as low as 1 keV. Despite a strong enhancement in the calculated event rate at low energies, we find that an interpretation in terms of electron-interacting WIMPs cannot be consistent with ex…

DAMA/LIBRACosmology and Nongalactic Astrophysics (astro-ph.CO)detector: performancePhysics::Instrumentation and DetectorsDark matterFOS: Physical scienceschemistry.chemical_elementElectron01 natural sciencesWIMP: dark matterNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)XenonWIMP0103 physical sciences010306 general physicsenhancementscintillation counterenergy: lowPhysicsScintillationxenon: liquid010308 nuclear & particles physicsatom: wave functionDAMAmodulationHigh Energy Physics - Phenomenologychemistryelectron: scatteringWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]direct detection[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astrophysics and astroparticle physicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review
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The Walking Dead: Cross-Channel connections and Funerary Practices c. 1600-1200 BC

2018

Session XXXII-4. Cross-channel connections from the Neolithic to the Bronze Age; International audience; The Middle /early Late Bronze Age (c. 1600-1200 BC) in the cross-channel region is invariably understood through the many close connections evidenced by new metal technologies and object types. These relationships tend to be interpreted as either continuities or developments from Early Bronze Age (c. 2200-1600 BC) cross-channel communities. However, whilst scholarship on the cross-channel connections between Early Bronze Age communities has tended to focus on funerary practices, there been no recent or comparable re-evaluation of cross-channel Middle /Late Bronze Age funerary practices. …

Bronze ageBritain[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistoryfunerary archaeologyFrance
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Parity-violating interactions of cosmic fields with atoms, molecules, and nuclei: Concepts and calculations for laboratory searches and extracting li…

2014

We propose methods and present calculations that can be used to search for evidence of cosmic fields by investigating the parity-violating effects, including parity nonconservation amplitudes and electric dipole moments, that they induce in atoms. The results are used to constrain important fundamental parameters describing the strength of the interaction of various cosmic fields with electrons, protons, and neutrons. Candidates for such fields are dark matter (including axions) and dark energy, as well as several more exotic sources described by standard-model extensions. Existing parity nonconservation experiments in Cs, Dy, Yb, and Tl are combined with our calculations to directly place …

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Nuclear TheoryAtomic Physics (physics.atom-ph)Dark matterFOS: Physical sciencesCosmic rayElectron01 natural sciencesPhysics - Atomic PhysicsNuclear physicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)Physics - Space Physics0103 physical sciencesNeutron010306 general physicsNuclear ExperimentPseudovectorPhysics010308 nuclear & particles physicsSpace Physics (physics.space-ph)PseudoscalarDipoleHigh Energy Physics - PhenomenologyNucleonAstrophysics - Cosmology and Nongalactic Astrophysics
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New Atomic Methods for Dark Matter Detection

2015

We calculate the parity and time-reversal violating effects that are induced in atoms, nuclei, and molecules by their interaction with various background cosmic fields, such as axion dark matter or dark energy.

PhysicsHistoryParticle physicsAxion Dark Matter ExperimentHot dark matterHigh Energy Physics::PhenomenologyDark matterScalar field dark matterAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science ApplicationsEducationMixed dark matterWarm dark matterLight dark matterDark fluidJournal of Physics: Conference Series
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Ionization of atoms by slow heavy particles, including dark matter

2016

Atoms and molecules can become ionized during the scattering of a slow, heavy particle off a bound electron. Such an interaction involving leptophilic weakly interacting massive particles (WIMPs) is a promising possible explanation for the anomalous 9 sigma annual modulation in the DAMA dark matter direct detection experiment [R. Bernabei et al., Eur. Phys. J. C 73, 2648 (2013)]. We demonstrate the applicability of the Born approximation for such an interaction by showing its equivalence to the semiclassical adiabatic treatment of atomic ionization by slow-moving WIMPs. Conventional wisdom has it that the ionization probability for such a process should be exponentially small. We show, howe…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)010308 nuclear & particles physicsScatteringDark matterAtoms in moleculesFOS: Physical sciencesGeneral Physics and AstronomyElectron01 natural sciencesAstrophysics - Astrophysics of GalaxiesPhysics - Atomic PhysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics of Galaxies (astro-ph.GA)IonizationWeakly interacting massive particles0103 physical sciencesBorn approximationAtomic physics010306 general physicsRelativistic quantum chemistryAstrophysics - Cosmology and Nongalactic Astrophysics
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