0000000000256195

AUTHOR

Carsten Henkel

0000-0002-8468-7502

showing 4 related works from this author

Stern-Gerlach splitting of low-energy ion beams

2019

We present a feasibility study with several magnetic field configurations for creating spin-dependent forces that can split a low-energy ion beam by the Stern-Gerlach effect. To the best of our knowledge, coherent spin-splittings of charged particles have yet to be realised. Our proposal is based on ion source parameters taken from a recent experiment that demonstrated single-ion implantation from a high-brightness ion source combined with a radio-frequency Paul trap. The inhomogeneous magnetic fields can be created by permanently magnetised microstructures or from current-carrying wires with sizes in the micron range, such as those recently used in a successful implementation of the Stern-…

PhysicsQuantum PhysicsStern–Gerlach experimentIon beamAtomic Physics (physics.atom-ph)Institut für Physik und AstronomieGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesIon sourceCharged particlePhysics - Atomic Physics010305 fluids & plasmasMagnetic fieldIonsymbols.namesake0103 physical sciencessymbolsddc:530Ion trapAtomic physics010306 general physicsQuantum Physics (quant-ph)Lorentz force
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Detection of deuterated molecules, but not of lithium hydride, in the z = 0.89 absorber toward PKS 1830−211

2020

Deuterium and lithium are light elements of high cosmological and astrophysical importance. In this work we report the first detection of deuterated molecules and a search for lithium hydride, 7LiH, at redshift z=0.89 in the spiral galaxy intercepting the line of sight to the quasar PKS1830-211. We used ALMA to observe several submillimeter lines of ND, NH2D, and HDO, and their related isotopomers NH2, NH3, and H2^18O, in absorption against the southwest image of the quasar, allowing us to derive XD/XH abundance ratios. The absorption spectra mainly consist of two distinct narrow velocity components for which we find remarkable differences. One velocity component shows XD/XH abundances that…

Absorption spectroscopyquasarsFOS: Physical scienceschemistry.chemical_elementAstrophysics01 natural scienceschemistry.chemical_compound0103 physical sciencesISM -galaxiesgalaxiesindividual010303 astronomy & astrophysicsLine (formation)Physics[PHYS]Physics [physics]Spiral galaxy010308 nuclear & particles physicsmolecules -radio linesAstronomy and AstrophysicsQuasarAstrophysics - Astrophysics of GalaxiesRedshift3. Good healthPKS 1830−211 -galaxiesabundances -ISMDeuteriumchemistry13. Climate actionSpace and Planetary ScienceLithium hydride[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Lithium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorption lines -quasars
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Dynamical Casimir-Polder interaction between an atom and surface plasmons

2013

We investigate the time-dependent Casimir-Polder potential of a polarizable two-level atom placed near a surface of arbitrary material, after a sudden change in the parameters of the system. Different initial conditions are taken into account. For an initially bare ground-state atom, the time-dependent Casimir-Polder energy reveals how the atom is "being dressed" by virtual, matter-assisted photons. We also study the transient behavior of the Casimir-Polder interaction between the atom and the surface starting from a partially dressed state, after an externally induced change in the atomic level structure or transition dipoles. The Heisenberg equations are solved through an iterative techni…

PhysicsCondensed Matter::Quantum GasesQuantum PhysicsSurface plasmons.Surface plasmonInstitut für Physik und AstronomieFOS: Physical sciencesInteraction energySurface plasmon polaritonAtomic and Molecular Physics and OpticsDynamical Casimir-Polder interactionCasimir effectAtom laserAtomic electron transitionQuantum mechanicsAtomQuasiparticlePhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsQuantum Physics (quant-ph)
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Temperature dependence of the magnetic Casimir-Polder interaction

2009

We analyze the magnetic dipole contribution to atom-surface dispersion forces. Unlike its electrical counterpart, it involves small transition frequencies that are comparable to thermal energy scales. A significant temperature dependence is found near surfaces with a nonzero DC conductivity, leading to a strong suppression of the dispersion force at T > 0. We use thermal response theory for the surface material and discuss both normal metals and superconductors. The asymptotes of the free energy of interaction and of the entropy are calculated analytically over a large range of distances. Near a superconductor, the onset of dissipation at the phase transition strongly changes the interac…

SuperconductivityPhysicsQuantum PhysicsPhase transitionMagnetic momentCondensed matter physicsFOS: Physical sciencesDissipationLondon dispersion forceAtomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterCasimir effectDipoleCasimir-Polder force Casimir effect dispersion forcesQuantum Physics (quant-ph)Magnetic dipoleOther Condensed Matter (cond-mat.other)Physical Review A
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