dorsal/arxiv
View SchemaOn the relativistic field theory model of the deuteron II
| Authors | A. N. Ivanov, N. I. Troitskaya, M. Faber, H. Oberhummer |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9704031 |
| URL | https://arxiv.org/abs/nucl-th/9704031 |
| DOI | 10.1016/S0375-9474(97)00016-X |
| Journal | Nucl.Phys.A617:414-448,1997; Erratum-ibid.A618:509,1997; Erratum-ibid.A625:896-898,1997 |
Abstract
The relativistic field theory model of the deuteron is applied to the calculation of the cross sections of the low-energy radiative neutron-proton capture n + p -> D + gamma and the low-energy two-proton fusion p + p -> D + e^+ + nu_e. For the low-energy radiative neutron-proton capture n + p -> D + gamma our result agrees well with both the experimental data and the potential model prediction. In the case of the two-proton fusion the cross section obtained is 2.9 times as much as that given by the potential approach. The obtained result is discussed in connection with the solar neutrino problem. ERRATUM: We correct the value of the cross section for pp-fusion p + p -> D + e^+ + nu_e. We find a contribution to the astrophysical factor \delta S_pp(0) = 2.01 x 10^{-25} (1 +/- 0.30) MeV b which is obtained only due to weak and strong low-energy interactions of the protons and the deuteron when neglecting the Coulomb repulsion between protons in the intermediate state. Minor misprints are corrected.
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"abstract": "The relativistic field theory model of the deuteron is applied to the\ncalculation of the cross sections of the low-energy radiative neutron-proton\ncapture n + p -\u003e D + gamma and the low-energy two-proton fusion p + p -\u003e D +\ne^+ + nu_e. For the low-energy radiative neutron-proton capture n + p -\u003e D +\ngamma our result agrees well with both the experimental data and the potential\nmodel prediction. In the case of the two-proton fusion the cross section\nobtained is 2.9 times as much as that given by the potential approach. The\nobtained result is discussed in connection with the solar neutrino problem.\n ERRATUM: We correct the value of the cross section for pp-fusion p + p -\u003e D +\ne^+ + nu_e. We find a contribution to the astrophysical factor \\delta S_pp(0) =\n2.01 x 10^{-25} (1 +/- 0.30) MeV b which is obtained only due to weak and\nstrong low-energy interactions of the protons and the deuteron when neglecting\nthe Coulomb repulsion between protons in the intermediate state. Minor\nmisprints are corrected.",
"arxiv_id": "nucl-th/9704031",
"authors": [
"A. N. Ivanov",
"N. I. Troitskaya",
"M. Faber",
"H. Oberhummer"
],
"categories": [
"nucl-th",
"astro-ph"
],
"doi": "10.1016/S0375-9474(97)00016-X",
"journal_ref": "Nucl.Phys.A617:414-448,1997; Erratum-ibid.A618:509,1997;\n Erratum-ibid.A625:896-898,1997",
"title": "On the relativistic field theory model of the deuteron II",
"url": "https://arxiv.org/abs/nucl-th/9704031"
},
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