Zobrazeno 1 - 10
of 16
pro vyhledávání: '"J. K. Bøggild"'
Autor:
L. Scarsi, L. Crane, A. Milone, G. Tomasini, M. Di Corato, J. H. Davies, D. Evans, T. E. Nevin, C. F. Powell, F. Anderson, M. Merlin, M. Grilli, N. Brene, M. G. K. Menon, A. Bonetti, R. Hillier, J. K. Bøggild, P. H. Fowler, B. Sechi, G. A. Salandin, M. Scharff, M. Ceccarelli, M. W. Friedlander, D. Keefe, J. E. Hooper, R. Levi Setti, W. C. G. Ortel, R.H.W. Johnston, P. E. Francois, G. P. S. Occhialini, P. Iredale, D. H. Perkins, C. O'Ceallaigh, G. Alvial, G. Lawlor, Constance Dilworth
Publikováno v:
Il Nuovo Cimento. 2:1063-1103
A large emulsion stack, exposed at high altitude, has been used to study the decaymodes of K-particles which produce a single charged secondary. The 5 decay modes, K μ , χ, ϰ and τ′ have been recognized from the nature and energy of the charged
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2a86d5d4031cda5df7350950bfa0d8a1
https://doi.org/10.1007/bf02855853
https://doi.org/10.1007/bf02855853
Autor:
M. Scharff, J. K. Bøggild
Publikováno v:
Il Nuovo Cimento. 12:374-380
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad1e8aba911061dc9e3b944c6ffce25c
https://doi.org/10.1007/bf02781532
https://doi.org/10.1007/bf02781532
Publikováno v:
Il Nuovo Cimento. 26:305-335
The process of slo~Sng down of charged par t ic les in m a t t e r is s tudied p a r t l y because of the intr insic in teres t of the processes invo lved and p a r t l y because knowledge of this p h e n o m e n o n has become an i m p o r t a n t t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b5b522c501daa5320a2ed636d0f1eb22
https://doi.org/10.1007/bf02782168
https://doi.org/10.1007/bf02782168
Autor:
L. Minnhagen, J. K. Bøggild
Publikováno v:
Physical Review. 75:782-785
The ranges of tritons and alpha-particles formed in the slow neutron reaction $^{6}\mathrm{Li}(n,\ensuremath{\alpha})^{3}\mathrm{H}$ have been measured in a cloud chamber and found to be ${R}_{\ensuremath{\alpha}}=10.4\ifmmode\pm\else\textpm\fi{}0.2$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c05c56dd00cbf749c06c56df78ec3b1a
https://doi.org/10.1103/physrev.75.782
https://doi.org/10.1103/physrev.75.782
Autor:
J. K. Bøggild
Publikováno v:
Physical Review. 60:827-830
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6d522e881b680c9116c7251e2d8e060f
https://doi.org/10.1103/physrev.60.827
https://doi.org/10.1103/physrev.60.827
Publikováno v:
Il Nuovo Cimento. 19:621-641
K+-decay events in a large block of emulsions have been studied, mainly by following the charged secondaries to the ends of their ranges. Emphasis was laid on: 1) obtaining unbiassed information on the high energy end of the spectrum of the Kμ3 seco
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0d6d0a2ebca6cc399675b3f4bac70840
https://doi.org/10.1007/bf02733361
https://doi.org/10.1007/bf02733361
Publikováno v:
Il Nuovo Cimento. 12:223-226
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a5012afc7187336f540a8c3cd5a9361d
https://doi.org/10.1007/bf02781489
https://doi.org/10.1007/bf02781489
Publikováno v:
Il Nuovo Cimento. 8:767-769
The pi - mu -e decay was studied in a stack of photographic emulsiohs exposed to cosmic radiation. Part of thin stack had earlier been scanned for mesonic events. The decays observsd, 796, fulfilled the requirements that the mu -meson stop more than
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7c9a03e31e8043e7d8f7a2d274abc460
https://doi.org/10.1007/bf02815257
https://doi.org/10.1007/bf02815257
Publikováno v:
Physical Review. 58:651-653
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2465bb2f47dd8391cdd7e7ae963d7cf4
https://doi.org/10.1103/physrev.58.651
https://doi.org/10.1103/physrev.58.651
Publikováno v:
Physical Review. 59:275-277
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e7a69e1e502c391cd85a3369b8f9c28a
https://doi.org/10.1103/physrev.59.275
https://doi.org/10.1103/physrev.59.275