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Three charged particles in the continuum : Astrophysical examples. / Belyaev, V. B.; Levin, S. B.; Yakovlev, S. L.

In: Journal of Physics B: Atomic, Molecular and Optical Physics, Vol. 37, No. 6, 28.03.2004, p. 1369-1380.

Research output: Contribution to journal › Article › peer-review

Harvard

Belyaev, VB, Levin, SB & Yakovlev, SL 2004, 'Three charged particles in the continuum: Astrophysical examples', Journal of Physics B: Atomic, Molecular and Optical Physics, vol. 37, no. 6, pp. 1369-1380. https://doi.org/10.1088/0953-4075/37/6/018

APA

Belyaev, V. B., Levin, S. B., & Yakovlev, S. L. (2004). Three charged particles in the continuum: Astrophysical examples. Journal of Physics B: Atomic, Molecular and Optical Physics, 37(6), 1369-1380. https://doi.org/10.1088/0953-4075/37/6/018

Vancouver

Belyaev VB, Levin SB, Yakovlev SL. Three charged particles in the continuum: Astrophysical examples. Journal of Physics B: Atomic, Molecular and Optical Physics. 2004 Mar 28;37(6):1369-1380. https://doi.org/10.1088/0953-4075/37/6/018

Author

Belyaev, V. B. ; Levin, S. B. ; Yakovlev, S. L. / Three charged particles in the continuum : Astrophysical examples. In: Journal of Physics B: Atomic, Molecular and Optical Physics. 2004 ; Vol. 37, No. 6. pp. 1369-1380.

BibTeX

@article{e5d0749eb1264a98a4bc6428f6db33bd,
title = "Three charged particles in the continuum: Astrophysical examples",
abstract = "We suggest a new adiabatic approach for the description of three charged particles in the continuum. This approach is based on the Coulomb-Fourier transformation of a three-body Hamiltonian, which allows us to develop a scheme, alternative to the Born-Oppenheimer one. The approach appears as an expansion of the kernels of corresponding integral transformations in terms of small mass-ratio parameter. To be specific, the results are presented for the system ppe in the continuum. The wavefunction of such a system is compared with the one which is used for the estimation of the rate for triple reaction p + p + e → d + v, which takes place as a step of the pp-cycle in the centre of the Sun. The problem of microscopic screening for this particular reaction is discussed.",
author = "Belyaev, {V. B.} and Levin, {S. B.} and Yakovlev, {S. L.}",
year = "2004",
month = mar,
day = "28",
doi = "10.1088/0953-4075/37/6/018",
language = "English",
volume = "37",
pages = "1369--1380",
journal = "Journal of the European Optical Society Part B: Quantum Optics",
issn = "0953-4075",
publisher = "IOP Publishing Ltd.",
number = "6",

}

RIS

TY - JOUR

T1 - Three charged particles in the continuum

T2 - Astrophysical examples

AU - Belyaev, V. B.

AU - Levin, S. B.

AU - Yakovlev, S. L.

PY - 2004/3/28

Y1 - 2004/3/28

N2 - We suggest a new adiabatic approach for the description of three charged particles in the continuum. This approach is based on the Coulomb-Fourier transformation of a three-body Hamiltonian, which allows us to develop a scheme, alternative to the Born-Oppenheimer one. The approach appears as an expansion of the kernels of corresponding integral transformations in terms of small mass-ratio parameter. To be specific, the results are presented for the system ppe in the continuum. The wavefunction of such a system is compared with the one which is used for the estimation of the rate for triple reaction p + p + e → d + v, which takes place as a step of the pp-cycle in the centre of the Sun. The problem of microscopic screening for this particular reaction is discussed.

AB - We suggest a new adiabatic approach for the description of three charged particles in the continuum. This approach is based on the Coulomb-Fourier transformation of a three-body Hamiltonian, which allows us to develop a scheme, alternative to the Born-Oppenheimer one. The approach appears as an expansion of the kernels of corresponding integral transformations in terms of small mass-ratio parameter. To be specific, the results are presented for the system ppe in the continuum. The wavefunction of such a system is compared with the one which is used for the estimation of the rate for triple reaction p + p + e → d + v, which takes place as a step of the pp-cycle in the centre of the Sun. The problem of microscopic screening for this particular reaction is discussed.

UR - http://www.scopus.com/inward/record.url?scp=1842584001&partnerID=8YFLogxK

U2 - 10.1088/0953-4075/37/6/018

DO - 10.1088/0953-4075/37/6/018

M3 - Article

VL - 37

SP - 1369

EP - 1380

JO - Journal of the European Optical Society Part B: Quantum Optics

JF - Journal of the European Optical Society Part B: Quantum Optics

SN - 0953-4075

IS - 6

ER -

ID: 5131729