The isospin dependence of the nucleus–nucleus inelastic cross-section at high energy

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Title: The isospin dependence of the nucleus–nucleus inelastic cross-section at high energy
Authors: Rashdan, M.1, Farhan, A.M.2 afarhan_afarhan@yahoo.com, Hassib, E.3, Kareem, W. Abdel3
Source: Chaos, Solitons & Fractals. May2006, Vol. 28 Issue 4, p1076-1081. 6p.
Subjects: Isobaric spin, Scattering (Mathematics), Integrals, Probability theory
Abstract: Abstract: The isospin dependence of the nucleus–nucleus inelastic cross-section at high energy is investigated within the multiple scattering theory. The multiple integrals are evaluated by Monte Carlo method as well as by the optical limit approximation of the Glauber model. Calculations are performed for 14–23N, 16–24O and 18–26F isotopes colliding with carbon target around 1GeV. It is found that rms radii and the density distributions show a halo structure of 22N, 23O and 24F. [Copyright &y& Elsevier]
Copyright of Chaos, Solitons & Fractals is the property of Pergamon Press - An Imprint of Elsevier Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: The isospin dependence of the nucleus–nucleus inelastic cross-section at high energy
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  Data: <searchLink fieldCode="AR" term="%22Rashdan%2C+M%2E%22">Rashdan, M.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Farhan%2C+A%2EM%2E%22">Farhan, A.M.</searchLink><relatesTo>2</relatesTo><i> afarhan_afarhan@yahoo.com</i><br /><searchLink fieldCode="AR" term="%22Hassib%2C+E%2E%22">Hassib, E.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Kareem%2C+W%2E+Abdel%22">Kareem, W. Abdel</searchLink><relatesTo>3</relatesTo>
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  Data: <searchLink fieldCode="JN" term="%22Chaos%2C+Solitons+%26+Fractals%22">Chaos, Solitons & Fractals</searchLink>. May2006, Vol. 28 Issue 4, p1076-1081. 6p.
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  Data: <searchLink fieldCode="DE" term="%22Isobaric+spin%22">Isobaric spin</searchLink><br /><searchLink fieldCode="DE" term="%22Scattering+%28Mathematics%29%22">Scattering (Mathematics)</searchLink><br /><searchLink fieldCode="DE" term="%22Integrals%22">Integrals</searchLink><br /><searchLink fieldCode="DE" term="%22Probability+theory%22">Probability theory</searchLink>
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  Data: Abstract: The isospin dependence of the nucleus–nucleus inelastic cross-section at high energy is investigated within the multiple scattering theory. The multiple integrals are evaluated by Monte Carlo method as well as by the optical limit approximation of the Glauber model. Calculations are performed for 14–23N, 16–24O and 18–26F isotopes colliding with carbon target around 1GeV. It is found that rms radii and the density distributions show a halo structure of 22N, 23O and 24F. [Copyright &y& Elsevier]
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  Data: <i>Copyright of Chaos, Solitons & Fractals is the property of Pergamon Press - An Imprint of Elsevier Science and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1016/j.chaos.2005.08.136
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        Text: English
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      – SubjectFull: Scattering (Mathematics)
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      – SubjectFull: Integrals
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      – TitleFull: The isospin dependence of the nucleus–nucleus inelastic cross-section at high energy
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