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Neutron production in Thunderstorms:
Neutron production in Thunderstorms:


The theory has been discussed as a theory to explain neutron production in thunderstorms,<ref name="Pramana" /> however, unreal concentrations of free electrons would be needed for the e–(p+, n)νe neutron yield to be a significant component of thunderstorm neutrons.<ref name="PRD">{{Cite journal |last=Babich |first=L P |last2=Bochkov |first2=E I |last3=Kutsyk |first3=I M |last4=Rassoul |first4=H K |title=Analysis of fundamental interactions capable of producing neutrons in thunderstorms |url=https://journals.aps.org/prd/abstract/10.1103/PhysRevD.89.093010#fulltext |journal=Physics Review D |publication-date=13 May 2014 |doi=https://doi.org/10.1103/PhysRevD.89.093010 |archive-url=https://dspace-test.lib.fit.edu/xmlui/bitstream/handle/11141/305/PRD20141D.pdf?sequence=1&isAllowed=y |archive-date=2014 |access-date=24 March 2017}}</ref>
The theory has been discussed as a theory to explain neutron production in thunderstorms,<ref name="Pramana" /> however, unreal concentrations of free electrons would be needed for the e–(p+, n)νe neutron yield to be a significant component of thunderstorm neutrons.<ref name="PRD">{{Cite journal |last=Babich |first=L P |last2=Bochkov |first2=E I |last3=Kutsyk |first3=I M |last4=Rassoul |first4=H K |title=Analysis of fundamental interactions capable of producing neutrons in thunderstorms |url=https://journals.aps.org/prd/abstract/10.1103/PhysRevD.89.093010#fulltext |journal=Physics Review D |publication-date=13 May 2014 |doi=10.1103/PhysRevD.89.093010 |archive-url=https://dspace-test.lib.fit.edu/xmlui/bitstream/handle/11141/305/PRD20141D.pdf?sequence=1&isAllowed=y |archive-date=2014 |access-date=24 March 2017}}</ref>
https://link.springer.com/article/10.1134/S1063776114030017
https://link.springer.com/article/10.1134/S1063776114030017
::http://crd.yerphi.am/files/Exploration-Discovery/Babich_Neutrons14.pdf
::http://crd.yerphi.am/files/Exploration-Discovery/Babich_Neutrons14.pdf

Revision as of 22:47, 23 March 2017

The Widom-Larsen theory is a theory developed by Dr. Axxxx Widom and Dr. Lxxxx Larsen which describes the production of ultra low momentum neutrons and subsequent catalysis of Low Energy Nuclear Reactions (LENR). The neutrons are hypothesized to be produced during weak interactions when protons capture "heavy" electrons in certain special conditions, such as metallic hydride surfaces.[1] The theory was expanded by Dr. Yogendra Srivastava, and additionally theorized as a possible explanation for neutrons observed in exploding wire experiments and thunderstorms.[2]


reliable secondary sources: https://www.researchgate.net/profile/Einar_Tennfors/publication/260246109_On_the_idea_of_low_energy_nuclear_reactions_in_metallic_lattices_by_producing_neutrons_from_protons_capturing_heavy_electrons/links/0f3175304c0ac9f4e3000000.pdf


Neutron production in Thunderstorms:

The theory has been discussed as a theory to explain neutron production in thunderstorms,[2] however, unreal concentrations of free electrons would be needed for the e–(p+, n)νe neutron yield to be a significant component of thunderstorm neutrons.[3] https://link.springer.com/article/10.1134/S1063776114030017

http://crd.yerphi.am/files/Exploration-Discovery/Babich_Neutrons14.pdf

https://journals.aps.org/prc/abstract/10.1103/PhysRevC.92.044602

http://crd.yerphi.am/files/Publication/References_to_CRD/Babich_anti_n20.pdf


References

  1. ^ Widom, A; Larsen, L (April 2006). "Ultra Low Momentum Neutron Catalyzed Nuclear Reactions on Metallic Hydride Surfaces" (PDF). The European Physical Journal C. doi:10.1140/epjc/s2006-02479-8. Archived from the original on 2 May 2005. Retrieved 24 March 2017.
  2. ^ a b Srivastava, Y; Widom, A; Larsen, L (October 2014). "A primer for electroweak induced low-energy nuclear reactions". Pramana – Journal of Physics. Retrieved 24 March 2017.
  3. ^ Babich, L P; Bochkov, E I; Kutsyk, I M; Rassoul, H K (13 May 2014). "Analysis of fundamental interactions capable of producing neutrons in thunderstorms" (PDF). Physics Review D. doi:10.1103/PhysRevD.89.093010. Archived from the original on 2014. Retrieved 24 March 2017. {{cite journal}}: Check date values in: |archive-date= (help)