A method for detecting the possible existence of high energy deuterons in the primary cosmic radiation
- 1 September 1960
- journal article
- Published by Springer Nature in Il Nuovo Cimento (1869-1876)
- Vol. 17 (6) , 837-844
- https://doi.org/10.1007/bf02732126
Abstract
No abstract availableKeywords
This publication has 9 references indexed in Scilit:
- Heavy Nuclei andαParticles between 7 and 100 Bev/Nucleon. I. Interaction Mean Free Paths and Fragmentation ProbabilitiesPhysical Review B, 1959
- On the origin of the charge spectrum of the primary cosmic radiationIl Nuovo Cimento (1869-1876), 1958
- Abundance of Light Nuclei in the Primary Cosmic RadiationPhysical Review B, 1958
- On the charge and energy spectrum of heavy primaries in cosmic radiationIl Nuovo Cimento (1869-1876), 1958
- Origin of Cosmic RaysProgress of Theoretical Physics Supplement, 1958
- The charge distribution of multiply charged nuclei in the primary cosmic radiation part I: The light and medium nucleiPhilosophical Magazine, 1957
- Nuclear disintegrations produced in nuclear emulsions by α-particles of great energyProceedings of the Indian Academy of Sciences - Section A, 1956
- Abundances of the ElementsReviews of Modern Physics, 1956
- On the nuclear interaction of 350 MeV α-particlesIl Nuovo Cimento (1869-1876), 1955