Condensed matter effects in the solar neutrino problem
| ISSN: |
1572-9575
|
|---|---|
| Source: |
Springer Online Journal Archives 1860-2000
|
| Topics: |
Physics
|
| Notes: |
Abstract In addition to our earlier corrections to fusion cross sections, we proposed that previously overlooked condensed matter effects (CME) can help to account for the missing solar neutrino flux. There are three important CME. One is due to a reduction in collision frequency due to an exchange of kinetic and potential energies in collision processes. Another is an excluded volume effect. The third is a shadowing effect due to the presence of spectator species which do not participate in fusion. These CME become appreciable in the high densities encountered in stellar media where they significantly affect fusion rates, since the solar core plasma cannot accurately be described as a collisionless ideal gas. Contrary to Bahcall and Gould (1993), we do not violate Liouville's theorem, the Maxwellian distribution, nor thermodynamics in our proposed solution to the solar neutrino problem.
|
| Type of Medium: |
Electronic Resource
|
| URL: |
| _version_ | 1798296481124319232 |
|---|---|
| autor | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. |
| autorsonst | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. |
| book_url | http://dx.doi.org/10.1007/BF00675800 |
| datenlieferant | nat_lic_papers |
| hauptsatz | hsatz_simple |
| identnr | NLM19742810X |
| issn | 1572-9575 |
| journal_name | International journal of theoretical physics |
| materialart | 1 |
| notes | Abstract In addition to our earlier corrections to fusion cross sections, we proposed that previously overlooked condensed matter effects (CME) can help to account for the missing solar neutrino flux. There are three important CME. One is due to a reduction in collision frequency due to an exchange of kinetic and potential energies in collision processes. Another is an excluded volume effect. The third is a shadowing effect due to the presence of spectator species which do not participate in fusion. These CME become appreciable in the high densities encountered in stellar media where they significantly affect fusion rates, since the solar core plasma cannot accurately be described as a collisionless ideal gas. Contrary to Bahcall and Gould (1993), we do not violate Liouville's theorem, the Maxwellian distribution, nor thermodynamics in our proposed solution to the solar neutrino problem. |
| package_name | Springer |
| publikationsjahr_anzeige | 1994 |
| publikationsjahr_facette | 1994 |
| publikationsjahr_intervall | 8009:1990-1994 |
| publikationsjahr_sort | 1994 |
| publisher | Springer |
| reference | 33 (1994), S. 2189-2198 |
| search_space | articles |
| shingle_author_1 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. |
| shingle_author_2 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. |
| shingle_author_3 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. |
| shingle_author_4 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. |
| shingle_catch_all_1 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. Condensed matter effects in the solar neutrino problem Abstract In addition to our earlier corrections to fusion cross sections, we proposed that previously overlooked condensed matter effects (CME) can help to account for the missing solar neutrino flux. There are three important CME. One is due to a reduction in collision frequency due to an exchange of kinetic and potential energies in collision processes. Another is an excluded volume effect. The third is a shadowing effect due to the presence of spectator species which do not participate in fusion. These CME become appreciable in the high densities encountered in stellar media where they significantly affect fusion rates, since the solar core plasma cannot accurately be described as a collisionless ideal gas. Contrary to Bahcall and Gould (1993), we do not violate Liouville's theorem, the Maxwellian distribution, nor thermodynamics in our proposed solution to the solar neutrino problem. 1572-9575 15729575 Springer |
| shingle_catch_all_2 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. Condensed matter effects in the solar neutrino problem Abstract In addition to our earlier corrections to fusion cross sections, we proposed that previously overlooked condensed matter effects (CME) can help to account for the missing solar neutrino flux. There are three important CME. One is due to a reduction in collision frequency due to an exchange of kinetic and potential energies in collision processes. Another is an excluded volume effect. The third is a shadowing effect due to the presence of spectator species which do not participate in fusion. These CME become appreciable in the high densities encountered in stellar media where they significantly affect fusion rates, since the solar core plasma cannot accurately be described as a collisionless ideal gas. Contrary to Bahcall and Gould (1993), we do not violate Liouville's theorem, the Maxwellian distribution, nor thermodynamics in our proposed solution to the solar neutrino problem. 1572-9575 15729575 Springer |
| shingle_catch_all_3 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. Condensed matter effects in the solar neutrino problem Abstract In addition to our earlier corrections to fusion cross sections, we proposed that previously overlooked condensed matter effects (CME) can help to account for the missing solar neutrino flux. There are three important CME. One is due to a reduction in collision frequency due to an exchange of kinetic and potential energies in collision processes. Another is an excluded volume effect. The third is a shadowing effect due to the presence of spectator species which do not participate in fusion. These CME become appreciable in the high densities encountered in stellar media where they significantly affect fusion rates, since the solar core plasma cannot accurately be described as a collisionless ideal gas. Contrary to Bahcall and Gould (1993), we do not violate Liouville's theorem, the Maxwellian distribution, nor thermodynamics in our proposed solution to the solar neutrino problem. 1572-9575 15729575 Springer |
| shingle_catch_all_4 | Rabinowitz, M. Kim, Y. E. Yoon, J. -H. Condensed matter effects in the solar neutrino problem Abstract In addition to our earlier corrections to fusion cross sections, we proposed that previously overlooked condensed matter effects (CME) can help to account for the missing solar neutrino flux. There are three important CME. One is due to a reduction in collision frequency due to an exchange of kinetic and potential energies in collision processes. Another is an excluded volume effect. The third is a shadowing effect due to the presence of spectator species which do not participate in fusion. These CME become appreciable in the high densities encountered in stellar media where they significantly affect fusion rates, since the solar core plasma cannot accurately be described as a collisionless ideal gas. Contrary to Bahcall and Gould (1993), we do not violate Liouville's theorem, the Maxwellian distribution, nor thermodynamics in our proposed solution to the solar neutrino problem. 1572-9575 15729575 Springer |
| shingle_title_1 | Condensed matter effects in the solar neutrino problem |
| shingle_title_2 | Condensed matter effects in the solar neutrino problem |
| shingle_title_3 | Condensed matter effects in the solar neutrino problem |
| shingle_title_4 | Condensed matter effects in the solar neutrino problem |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Springer Online Journal Archives 1860-2000 |
| timestamp | 2024-05-06T09:52:45.903Z |
| titel | Condensed matter effects in the solar neutrino problem |
| titel_suche | Condensed matter effects in the solar neutrino problem |
| topic | U |
| uid | nat_lic_papers_NLM19742810X |