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arXiv:physics/0612050 · Physical Review A

Interaction of ultracold antihydrogen with a conducting wall

Alexei Yu. Voronin, Piotr Froelich, Bernard Zygelman

Published Dec 29, 2005• 76 citations
arXivHTMLPDF

Abstract

We investigate the interaction of ultracold antihydrogen with a conducting surface, focusing on the phenomenon of quantum reflection. We calculate the reflection probability as a function of incident atom energy. We find that, for ground-state $\overline{\mathrm{H}}$ atoms (with $T<{10}^{\ensuremath{-}5}\phantom{\rule{0.3em}{0ex}}\mathrm{K})$, the probability of reflection is $R\ensuremath{\simeq}1\ensuremath{-}kb$, where $k$ is the momentum of the atom and $b=2174.0\phantom{\rule{0.3em}{0ex}}\mathrm{a}.\mathrm{u}.$ is a constant determined solely by the van der Waals--Casimir tail of the atom-wall interaction. We show that quantum reflection, which suppresses the direct contact of ultracold atoms with the surface, allows for the possibility of confinement and storage of sufficiently cold antihydrogen atoms. We calculate the lifetime of $\overline{\mathrm{H}}$ atoms enclosed in between solid walls. We develop a theory of $\overline{\mathrm{H}}$ in a waveguide and propose some applications, notably the measurement of retardation corrections in the long-range component of the antiatom-wall potential. We demonstrate the existence of quantized states for antihydrogen atoms falling onto conducting surface in the gravitational field of Earth. We calculate the lifetime of ultracold $\overline{\mathrm{H}}$ in its lowest gravitational state and obtain $\ensuremath{\tau}=(Mgb∕2\ensuremath{\Elzxh}{)}^{\ensuremath{-}1}\ensuremath{\simeq}0.1\phantom{\rule{0.3em}{0ex}}\mathrm{s}$, where $Mg$ is a gravitational force acting on the antiatom. We propose that measurement of this lifetime may provide a new test for the gravitational properties of antimatter.

DOI
10.1103/physreva.72.062903

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We investigate the interaction of ultracold antihydrogen with a conducting surface, focusing on the phenomenon of quantum reflection. We calculate the reflection probability as a function of incident atom energy. We find that, for ground-state H‾\overline{\mathrm{H}}H atoms (with T<10\ensuremath−5K)T<{10}^{\ensuremath{-}5}\phantom{\rule{0.3em}{0ex}}\mathrm{K})T<10\ensuremath−5K), the probability of reflection is R\ensuremath≃1\ensuremath−kbR\ensuremath{\simeq}1\ensuremath{-}kbR\ensuremath≃1\ensuremath−kb, where kkk is the momentum of the atom and b=2174.0a.u.b=2174.0\phantom{\rule{0.3em}{0ex}}\mathrm{a}.\mathrm{u}.b=2174.0a.u. is a constant determined solely by the van der Waals--Casimir tail of the atom-wall interaction. We show that quantum reflection, which suppresses the direct contact of ultracold atoms with the surface, allows for the possibility of confinement and storage of sufficiently cold antihydrogen atoms. We calculate the lifetime of H‾\overline{\mathrm{H}}H atoms enclosed in between solid walls. We develop a theory of H‾\overline{\mathrm{H}}H in a waveguide and propose some applications, notably the measurement of retardation corrections in the long-range component of the antiatom-wall potential. We demonstrate the existence of quantized states for antihydrogen atoms falling onto conducting surface in the gravitational field of Earth. We calculate the lifetime of ultracold H‾\overline{\mathrm{H}}H in its lowest gravitational state and obtain \ensuremathτ=(Mgb∕2\ensuremath\Elzxh)\ensuremath−1\ensuremath≃0.1s\ensuremath{\tau}=(Mgb∕2\ensuremath{\Elzxh}{)}^{\ensuremath{-}1}\ensuremath{\simeq}0.1\phantom{\rule{0.3em}{0ex}}\mathrm{s}\ensuremathτ=(Mgb∕2\ensuremath\Elzxh)\ensuremath−1\ensuremath≃0.1s, where MgMgMg is a gravitational force acting on the antiatom. We propose that measurement of this lifetime may provide a new test for the gravitational properties of antimatter.
We consider the interaction of antiatoms with a solid surface and present calculations of the reflection probability using the exact retarded potential for the antihydrogen impinging on the ideally conducting surface. We present the reflection probability as a function of collision energy and show that the sufficiently cold ¯ H atoms are reflected (rather than annihilated) from the surface, which opens prospects for storing and guiding antiatoms between material walls. The reflection probability in the ultracold regime is determined entirely by the van der Waals–Casimir tail of the atom–wall interaction and contains information on the retardation effects. We argue on the possibility of exploiting the ultracold antihydrogen–surface interactions as a probe of the electrodynamical and gravitational properties of an antiatom. We found that the lifetime of cold ¯ H bouncing on the surface in the gravitational field of Earth is τ = ¯2Mg|Im a|) � 0.11 s. The measurement of that lifetime in conjunction with our calculation of the scattering lengtha allows determination of the gravitational force Mg on the antihydrogen atom.
We show that the ultracold H̄ atoms below 10−6 K are reflected from the surface with the probability , which is determined entirely by the van der Waals‐Casimir tail of the atom‐wall interaction and contains information on the retardation effects. We found, that the lifetime of cold H̄ bouncing on the conducting surface in the gravitational field of Earth is τ = ℏ/(2Mg|Ima|) ≃ 0.11 s. The measurement of that lifetime in conjunction with the here presented calculation of the scattering length a allows determination of the gravitational force Mg acting on the antihydrogen atom.
In the GBAR experiment, cold antihydrogen atoms will be left to fall on an annihilation plate with the aim of measuring the gravitational acceleration of antimatter. Here, we study the quantum reflection of these antiatoms due to the Casimir-Polder potential above the plate. We give realistic estimates of the potential and quantum reflection amplitudes, taking into account the specificities of antihydrogen and the optical properties of the plate. We find that quantum reflection is enhanced for weaker potentials, for example above thin slabs, graphene and nanoporous media.
We study quantum reflection of antihydrogen atoms from matter slabs due to the van der Waals--Casimir-Polder potential. By taking into account the specificities of antihydrogen and the optical properties and width of the slabs, we calculate realistic estimates for the potential and quantum reflection amplitudes. Next we discuss the paradoxical result of larger reflection coefficients estimated for weaker potentials in terms of the Schwarzian derivative. We analyze the limiting case of reflections at small energies, which are characterized by a scattering length and have interesting applications for trapping and guiding antihydrogen using material walls.
Collisions between ultracold atoms and material surfaces are characterized by the reflection of the atomic matter wave from the attractive Casimir-Polder potential. This quantum reflection is particularly relevant to experiments such as GBAR, which will determine the gravitational acceleration of a cold antihydrogen atom by timing its fall onto a detection plate. In this thesis, the Casimir-Polder potential is computed from the electromagnetic scattering properties of the atom and surface and it is found to depend notably on the dielectric response, thickness and density of the medium. We show that reflection on this potential is associated with a breakdown of the semiclassical approximation and that it is enhanced for slow atoms and weak potentials. Liouville transformations relate Schrödinger equations with different potential landscapes but identical scattering properties. We gain new insights on the problem of quantum reflection on a potential well by mapping it onto an equivalent problem of tunneling through a wall. We also discuss the effect of gravity on the atomic wavepacket and its implications for free fall experiments with atoms. When combined with quantum reflection from a horizontal mirror, gravity can be used to trap particles in long lived states with promising applications for metrology. In particular, we suggest a scheme to improve the precision of the GBAR experiment by reducing the velocity dispersion of the falling atoms.
We present a theoretical study of the motion of the antihydrogen atom (H‾\overline{\mathrm{H}}H) in the gravitational field of Earth above a material surface. We predict that the H‾\overline{\mathrm{H}}H atom, falling in the gravitational field of Earth above a material surface, would settle into long-lived quantum states. We point out a method of measuring the difference in the energy of H‾\overline{\mathrm{H}}H in such states. The method allows for spectroscopy of gravitational levels based on atom-interferometric principles. We analyze the general feasibility of performing experiments of this kind. We point out that such experiments provide a method of measuring the gravitational force (Mg\mathit{Mg}Mg) acting on H‾\overline{\mathrm{H}}H and that they might be of interest in the context of testing the weak equivalence principle for antimatter.