dorsal/arxiv
View SchemaSum rule for the backward spin polarizability of the nucleon from a backward dispersion relation
| Authors | A. I. L'vov, A. M. Nathan |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9807032 |
| URL | https://arxiv.org/abs/nucl-th/9807032 |
| DOI | 10.1103/PhysRevC.59.1064 |
| Journal | Phys.Rev. C59 (1999) 1064-1069 |
Abstract
A new sum rule for $\gamma_\pi$, the backward spin polarizability of the nucleon, is derived from a backward-angle dispersion relation. Taking into account single- and multi-pion photoproduction in the s-channel up to the energy 1.5 GeV and resonances in the t-channel with mass below 1.5 GeV, it is found for the proton and neutron that $[\gamma_\pi]_p$ = -39.5 +/- 2.4 and $[\gamma_\pi]_n$ = 52.5 +/- 2.4, respectively, in units of 10^{-4} fm^4.
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"abstract": "A new sum rule for $\\gamma_\\pi$, the backward spin polarizability of the\nnucleon, is derived from a backward-angle dispersion relation. Taking into\naccount single- and multi-pion photoproduction in the s-channel up to the\nenergy 1.5 GeV and resonances in the t-channel with mass below 1.5 GeV, it is\nfound for the proton and neutron that $[\\gamma_\\pi]_p$ = -39.5 +/- 2.4 and\n$[\\gamma_\\pi]_n$ = 52.5 +/- 2.4, respectively, in units of 10^{-4} fm^4.",
"arxiv_id": "nucl-th/9807032",
"authors": [
"A. I. L\u0027vov",
"A. M. Nathan"
],
"categories": [
"nucl-th"
],
"doi": "10.1103/PhysRevC.59.1064",
"journal_ref": "Phys.Rev. C59 (1999) 1064-1069",
"title": "Sum rule for the backward spin polarizability of the nucleon from a backward dispersion relation",
"url": "https://arxiv.org/abs/nucl-th/9807032"
},
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