0000000000964801

AUTHOR

K. Miller

showing 6 related works from this author

Extrakorporale Stoßwellenlithotripsie (ESWL) — Physikalische und biologische Grundlagen

1988

Sieben Jahre sind inzwischen seit der ersten humanen ESWL-Behandlung im Februar 1980 vergangen, vier Jahre seit der Inbetriebnahme der 2. ESWL-Anlage hier in Stuttgart und damit seit dem Beginn der serienmasigen Verteilung der ESWL-Technologie, zunachst in der Bundesrepublik Deutschland, danach weltweit.

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Constraining the spin-dependent WIMP-nucleon cross sections with XENON1T

2019

We report the first experimental results on spin-dependent elastic weakly interacting massive particle (WIMP) nucleon scattering from the XENON1T dark matter search experiment. The analysis uses the full ton year exposure of XENON1T to constrain the spin-dependent proton-only and neutron-only cases. No significant signal excess is observed, and a profile likelihood ratio analysis is used to set exclusion limits on the WIMP-nucleon interactions. This includes the most stringent constraint to date on the WIMP-neutron cross section, with a minimum of 6.3 × 10−42 cm2 at 30 GeV/c2 and 90% confidence level. The results are compared with those from collider searches and used to exclude new paramet…

WIMP nucleon: interactionWIMP nucleon: scatteringParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)IsoscalarDark matterNuclear TheoryMassive particleGeneral Physics and AstronomyFOS: Physical sciencesParameter spacedark matter: direct detectionGravitation and Astrophysicsspin: dependence01 natural scienceslaw.inventionHigh Energy Physics - Phenomenology (hep-ph)WIMPlawisoscalar0103 physical sciencesS046DM1mediation010306 general physicsColliderPseudovectorPhysicsS030DN2S030DN1S030DP3S030DN3S030DP2S030DP1WIMP nucleon: cross sectionaxial-vectorHigh Energy Physics - PhenomenologyWIMPs Spin Dependent Cross Sections Neutron Cross Sections Likelihood methoddark matter: scattering[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentNucleon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysicsexperimental results
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Der Ausguß-Stein — Kontroverse Therapiekonzepte und Langzeitergebnisse

1988

Die Extrakorporale Stoswellen-Lithotripsie ist fuhrende Behandlungsform fur die Mehrzahl der nichtabgangsfahigen Nierensteine geworden und hinsichtlich ihrer Indikationsstellung bei der Behandlung kleiner Nierenbecken — oder Kelchsteine unumstritten. Lediglich bei der Behandlung von Ausgussteinen variieren die therapeutischen Konzepte von Klinik zu Klinik teilweise noch erheblich und eine endgultige Beurteilung der verschiedenen Behandlungsprinzipien ist derzeit noch nicht sicher moglich, weil es an Langzeitbeobachtungen fehlt.

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First Results on the Scalar WIMP-Pion Coupling, Using the XENON1T Experiment

2018

We present first results on the scalar coupling of weakly interacting massive particles (WIMPs) to pions from 1 t yr of exposure with the XENON1T experiment. This interaction is generated when the WIMP couples to a virtual pion exchanged between the nucleons in a nucleus. In contrast to most nonrelativistic operators, these pion-exchange currents can be coherently enhanced by the total number of nucleons and therefore may dominate in scenarios where spin-independent WIMP-nucleon interactions are suppressed. Moreover, for natural values of the couplings, they dominate over the spin-dependent channel due to their coherence in the nucleus. Using the signal model of this new WIMP-pion channel, …

Nuclear TheoryPhysics::Instrumentation and DetectorsNuclear TheoryGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMPPions[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentS030UDMPhysicsStarke Wechselwirkung und exotische Kerne – Abteilung BlaumAstrophysics::Instrumentation and Methods for AstrophysicsnucleonsuppressionHigh Energy Physics - PhenomenologyWeakly interacting massive particlesmedicine.anatomical_structureWeakly interacting massive particlesNucleonCoherence (physics)Astrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesWIMP: massspin: dependenceGravitation and Astrophysicsoperator: nonrelativisticDark matter Particle dark matter Pions Weakly interacting massive particles Dark matter detectorsNuclear Theory (nucl-th)PionParticle dark matter0103 physical sciencesmedicineDark mattercross section: upper limit010306 general physicsCouplingDark matter detectorsnucleusScalar (physics)coherenceDark Matter WIMP-Pion coupling Xenon Direct seartch[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Nucleus
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Dark Matter Search Results from a One Ton-Year Exposure of XENON1T

2018

We report on a search for Weakly Interacting Massive Particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of $(1.30 \pm 0.01)$ t, resulting in a 1.0 t$\times$yr exposure. The energy region of interest, [1.4, 10.6] $\mathrm{keV_{ee}}$ ([4.9, 40.9] $\mathrm{keV_{nr}}$), exhibits an ultra-low electron recoil background rate of $(82\substack{+5 \\ -3}\textrm{ (sys)}\pm3\textrm{ (stat)})$ events/$(\mathrm{t}\times\mathrm{yr}\times\mathrm{keV_{ee}})$. No significant excess over background is found and a profile likelihood analysis parameterized in spatial and energy dimensions exclude…

Dark matterGeneral Physics and Astronomychemistry.chemical_elementS030DI5WIMP: massElectronParameter spacedark matter: direct detectionGravitation and AstrophysicsS030DI101 natural sciencesS030DI3S030DI2Nuclear physicsXenonRecoilWIMPelectron: recoil0103 physical sciencesS046DM2[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsnumerical calculationsDark Matter WIMP TPC XENON Direct searchPhysicsxenon: liquidTime projection chamber010308 nuclear & particles physicsbackgrounddark matter: massGran SassoWIMP nucleonchemistryWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]time projection chamber: xenon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Two-neutron correlations at small relative momenta in ^40Ar + ^197Au collisions at 60 MeV/nucleon

2000

Two-neutron correlation functions are measured in the 40Ar + 197Au reaction at 60 MeV/nucleon to study the space-time characteristics of neutron emitting sources. The source temperatures and velocities are deduced by fitting the single-neutron energy spectra with a three-source model. A comparison of the correlation data with the predictions of the model of moving sources and with the dynamical Landau-Vlasov model suggests the relevance of a multisource description. Particular care has been paid to the influence of the relative source abundance on the shape of the correlation function.

010302 applied physicsPhysicsNuclear and High Energy Physics010308 nuclear & particles physicsNuclear Theory[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesSpectral lineNuclear physicsCorrelation function (statistical mechanics)0103 physical sciencesnuclear physics; heavy ions; neutron interferometryNeutronNucleonNuclear Experiment
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