1992
DOI: 10.1103/physreva.45.7782
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Atomic core-polarization effects in metastable hadronic helium atoms

Abstract: A theoretical consideration is presented concerning the atomic core-polarization effect on the E1 transitions of large-I circular orbitals in hadronic helium atoms (e X He~+), where the e occupies the 1s orbital and the negative hadron (X ) occupies a large-1 circular orbital. The first-order mixing of the 2p electron configuration due to the repulsive e -X interaction gives rise to a substantial suppression (-3) of the E1 transitions, compared with a single-particle estimate, since the slowly moving particle… Show more

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Cited by 89 publications
(38 citation statements)
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“…Of course, there are also contributions from Auger decay and radiative processes that change v ϵ n − l − 1, but calculations for a single isolated atom suggest that these contributions are all less than 10% [22,[30][31][32]. According to this model, the intensity I 1 ͑t 1 ͒ of the first spike [which is proportional to the population P ͑39,35͒ ͑t 1 ͒], and the intensity I 2 ͑t 1 , t 2 ͒ of the second spike [which contains information about the feeding into state ͑39, 35͒ from ͑40, 36͒ between t 1 and t 2 ] follow the analytical functions, The population evolution of state ͑39, 35͒ was measured using the pulsed (closed circles) and continuous (triangles) antiproton beams (d).…”
Section: A Population Evolution Of Metastable States In the V = 3 Camentioning
confidence: 99%
See 1 more Smart Citation
“…Of course, there are also contributions from Auger decay and radiative processes that change v ϵ n − l − 1, but calculations for a single isolated atom suggest that these contributions are all less than 10% [22,[30][31][32]. According to this model, the intensity I 1 ͑t 1 ͒ of the first spike [which is proportional to the population P ͑39,35͒ ͑t 1 ͒], and the intensity I 2 ͑t 1 , t 2 ͒ of the second spike [which contains information about the feeding into state ͑39, 35͒ from ͑40, 36͒ between t 1 and t 2 ] follow the analytical functions, The population evolution of state ͑39, 35͒ was measured using the pulsed (closed circles) and continuous (triangles) antiproton beams (d).…”
Section: A Population Evolution Of Metastable States In the V = 3 Camentioning
confidence: 99%
“…(ii) Thermalization: the pHe + atom initially recoils with roughly the same momentum as the incoming antiproton, but cools down within picoseconds by colliding with the surrounding helium atoms. (iii) Metastable cascade: The antiproton cascades down through several metastable levels by making successive radiative transitions with lifetimes =1−2 s, these being primarily of the type ⌬n = ⌬ᐉ = −1 that keeps the vibrational quantum number v ϵ n − ᐉ −1 [30][31][32] constant. The states can therefore be grouped into the cascade sequences v =0,1,2,3.... (iv) Auger decay: The antiproton finally reaches a short-lived state, from which Auger decay to an ionic state occurs within a few nanoseconds [8,22,33].…”
Section: ͑1͒mentioning
confidence: 99%
“…A prominent and important feature of the theoretically calculated Auger rates is their drastic dependence on the lowest possible transition multipolarity L, which is equal to the *Present address: Center for Nuclear Study (CNS), University of minimum angular momentum carried away by the Auger electron [10,12]. The theoretical rates are approximated by a rough estimation…”
Section: Introductionmentioning
confidence: 99%
“…In particular, the Auger rates ␥ A , which are dominant in the total decay rate for some pHe + states, have been calculated by many theorists [10][11][12][13] over a period of more than 30 years. The latest calculations with complex coordinate rotation (CCR) method by Korobov [7] and Kino [9] yield both real and imaginary parts of the complex energy at the same time, and the both parts are expected to have absolute precisions of the same order.…”
Section: Introductionmentioning
confidence: 99%
“…Due to the almost classical localization of the antiproton wavefunction for large-n states, transitions with n > 1 are much slower than those with n = 1, because the larger transition energies E n for n > 1 are outweighed by a m uch smaller overlap integral hfjE1jii of initial and nal state wavefunctions 13 . In the molecular picture, this means that the familiar selection rule v = ( n l 1 ) = 0 ; 1 for radiative transitions between low-lying vibrational states of an ordinary diatomic molecule is reduced to v = 0 in the case of pHe + due to the large angular momentum 14 .…”
Section: Introductionmentioning
confidence: 99%