Conventional nuclear physics solution of the solar neutrino problem
| ISSN: |
1572-9575
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| Source: |
Springer Online Journal Archives 1860-2000
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| Topics: |
Physics
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| Notes: |
Abstract A basic and inherently simple alternative explanation of the solar neutrino problem is proposed based upon conventional nuclear physics. Our results for the tunneling factor, astrophysicalS-factor, and our resolution are compared with rather speculative solutions commonly attempted by accepting the customary ingredients of the standard solar model. We present a more realistic solution of nuclear Coulomb barrier tunneling together with a more precise parametric representation of the astrophysical functionS. We determineS from high-energy (〉100 keV)7Be(p, γ)8B experimental cross-section data using the new tunneling factor. This leads to a low-energy fusion cross section that is lower than previous estimates by ∼26–36%, decreasing the anticipated neutrino flux close to experimentally detected values. This may resolve the missing solar neutrino flux problem.
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| Type of Medium: |
Electronic Resource
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| URL: |
| _version_ | 1798296479863930882 |
|---|---|
| autor | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. |
| autorsonst | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. |
| book_url | http://dx.doi.org/10.1007/BF00673718 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLM197426719 |
| issn | 1572-9575 |
| journal_name | International journal of theoretical physics |
| materialart | 1 |
| notes | Abstract A basic and inherently simple alternative explanation of the solar neutrino problem is proposed based upon conventional nuclear physics. Our results for the tunneling factor, astrophysicalS-factor, and our resolution are compared with rather speculative solutions commonly attempted by accepting the customary ingredients of the standard solar model. We present a more realistic solution of nuclear Coulomb barrier tunneling together with a more precise parametric representation of the astrophysical functionS. We determineS from high-energy (〉100 keV)7Be(p, γ)8B experimental cross-section data using the new tunneling factor. This leads to a low-energy fusion cross section that is lower than previous estimates by ∼26–36%, decreasing the anticipated neutrino flux close to experimentally detected values. This may resolve the missing solar neutrino flux problem. |
| package_name | Springer |
| publikationsjahr_anzeige | 1993 |
| publikationsjahr_facette | 1993 |
| publikationsjahr_intervall | 8009:1990-1994 |
| publikationsjahr_sort | 1993 |
| publisher | Springer |
| reference | 32 (1993), S. 301-317 |
| search_space | articles |
| shingle_author_1 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. |
| shingle_author_2 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. |
| shingle_author_3 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. |
| shingle_author_4 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. |
| shingle_catch_all_1 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. Conventional nuclear physics solution of the solar neutrino problem Abstract A basic and inherently simple alternative explanation of the solar neutrino problem is proposed based upon conventional nuclear physics. Our results for the tunneling factor, astrophysicalS-factor, and our resolution are compared with rather speculative solutions commonly attempted by accepting the customary ingredients of the standard solar model. We present a more realistic solution of nuclear Coulomb barrier tunneling together with a more precise parametric representation of the astrophysical functionS. We determineS from high-energy (〉100 keV)7Be(p, γ)8B experimental cross-section data using the new tunneling factor. This leads to a low-energy fusion cross section that is lower than previous estimates by ∼26–36%, decreasing the anticipated neutrino flux close to experimentally detected values. This may resolve the missing solar neutrino flux problem. 1572-9575 15729575 Springer |
| shingle_catch_all_2 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. Conventional nuclear physics solution of the solar neutrino problem Abstract A basic and inherently simple alternative explanation of the solar neutrino problem is proposed based upon conventional nuclear physics. Our results for the tunneling factor, astrophysicalS-factor, and our resolution are compared with rather speculative solutions commonly attempted by accepting the customary ingredients of the standard solar model. We present a more realistic solution of nuclear Coulomb barrier tunneling together with a more precise parametric representation of the astrophysical functionS. We determineS from high-energy (〉100 keV)7Be(p, γ)8B experimental cross-section data using the new tunneling factor. This leads to a low-energy fusion cross section that is lower than previous estimates by ∼26–36%, decreasing the anticipated neutrino flux close to experimentally detected values. This may resolve the missing solar neutrino flux problem. 1572-9575 15729575 Springer |
| shingle_catch_all_3 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. Conventional nuclear physics solution of the solar neutrino problem Abstract A basic and inherently simple alternative explanation of the solar neutrino problem is proposed based upon conventional nuclear physics. Our results for the tunneling factor, astrophysicalS-factor, and our resolution are compared with rather speculative solutions commonly attempted by accepting the customary ingredients of the standard solar model. We present a more realistic solution of nuclear Coulomb barrier tunneling together with a more precise parametric representation of the astrophysical functionS. We determineS from high-energy (〉100 keV)7Be(p, γ)8B experimental cross-section data using the new tunneling factor. This leads to a low-energy fusion cross section that is lower than previous estimates by ∼26–36%, decreasing the anticipated neutrino flux close to experimentally detected values. This may resolve the missing solar neutrino flux problem. 1572-9575 15729575 Springer |
| shingle_catch_all_4 | Kim, Y. E. Rabinowitz, M. Yoon, J. -H. Rice, R. A. Conventional nuclear physics solution of the solar neutrino problem Abstract A basic and inherently simple alternative explanation of the solar neutrino problem is proposed based upon conventional nuclear physics. Our results for the tunneling factor, astrophysicalS-factor, and our resolution are compared with rather speculative solutions commonly attempted by accepting the customary ingredients of the standard solar model. We present a more realistic solution of nuclear Coulomb barrier tunneling together with a more precise parametric representation of the astrophysical functionS. We determineS from high-energy (〉100 keV)7Be(p, γ)8B experimental cross-section data using the new tunneling factor. This leads to a low-energy fusion cross section that is lower than previous estimates by ∼26–36%, decreasing the anticipated neutrino flux close to experimentally detected values. This may resolve the missing solar neutrino flux problem. 1572-9575 15729575 Springer |
| shingle_title_1 | Conventional nuclear physics solution of the solar neutrino problem |
| shingle_title_2 | Conventional nuclear physics solution of the solar neutrino problem |
| shingle_title_3 | Conventional nuclear physics solution of the solar neutrino problem |
| shingle_title_4 | Conventional nuclear physics solution of the solar neutrino problem |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Springer Online Journal Archives 1860-2000 |
| timestamp | 2024-05-06T09:52:46.116Z |
| titel | Conventional nuclear physics solution of the solar neutrino problem |
| titel_suche | Conventional nuclear physics solution of the solar neutrino problem |
| topic | U |
| uid | nat_lic_papers_NLM197426719 |