High-energy N particles in extensive air showers at 800 g/cm2

1968 ◽  
Vol 46 (10) ◽  
pp. S136-S141 ◽  
Author(s):  
B. K. Chatterjee ◽  
G. T. Murthy ◽  
S. Naranan ◽  
B. V. Sreekantan ◽  
M. V. Srinivasa Rao ◽  
...  

The results on high-energy N particles in EAS using a total absorption spectrometer for energy measurement are presented. They are compared with results from other experiments and calculations based upon plausible models of high energy interactions. (1) As expected, the NAP lateral distribution becomes steeper for particles of higher threshold energies. (2) Contrary to expectation, the lateral distribution becomes flatter with increasing shower size. The implication of this anomalous behavior in terms of interaction characteristics at energies > 1014 eV is briefly discussed. (3) For a given size, showers with steeper electron lateral distribution have more NAPs. (4) Except for the behavior of the lateral distribution as a function of size, all the other results can be explained in terms of models in which pT and inelasticity distributions are invariant and some fraction (~15%) of nucleon–antinucleon pair production is assumed.

1968 ◽  
Vol 46 (10) ◽  
pp. S13-S16 ◽  
Author(s):  
B. K. Chatterjee ◽  
G. T. Murthy ◽  
S. Naranan ◽  
K. Sivaprasad ◽  
B. V. Sreekantan ◽  
...  

Measurements have been made on high-energy muons (>220 GeV and >640 GeV) in extensive air showers in the size range 105–107 particles. Results on the energy spectrum, lateral spread (for Eμ > 220 GeV), and the dependence of the total number of muons on the shower size are given. The relation between the number of muons (Nμ) and the shower size (N) can be expressed as[Formula: see text]Assuming an exponential lateral distribution of high-energy muons, the average lateral spread of muons of energy >220 GeV has been found to be ~40 m.The results are compared with the predictions of the calculations done by Murthy et al. (1967).


1990 ◽  
Vol 68 (1) ◽  
pp. 41-48 ◽  
Author(s):  
D. K. Basak ◽  
S. K. Sarkar ◽  
N. Mukherjee ◽  
S. Sanyal ◽  
B. Ghosh ◽  
...  

The energy spectra and the lateral distribution of muons in cosmic-ray air showers, in the size range 104–106 particles as measured by two magnetic spectrographs each of full detection efficiency for muons in the energy range 2.5–500 GeV, are presented along with the derived muon size vs. shower size results. Comparisons with similar recent experimental data and calculations are given to infer the cosmic-ray primary composition.


1973 ◽  
Vol 106 (1) ◽  
pp. 189-200 ◽  
Author(s):  
J. Engler ◽  
W. Flauger ◽  
B. Gibbard ◽  
F. Mönnig ◽  
K. Runge ◽  
...  

1973 ◽  
Vol 108 (3) ◽  
pp. 541-550 ◽  
Author(s):  
M. Holder ◽  
E. Radermacher ◽  
A. Staude ◽  
P. Darriulat ◽  
J. Deutsch ◽  
...  

2014 ◽  
Vol 66 ◽  
pp. 10019 ◽  
Author(s):  
A.-A. Zakari-Issoufou ◽  
A. Porta ◽  
M. Fallot ◽  
A. Algora ◽  
J.L Tain ◽  
...  

2019 ◽  
Vol 201 ◽  
pp. 03002
Author(s):  
Michał Stepaniuk ◽  
Marek Karny ◽  
Aleksandra Fijałkowska ◽  
Wojciech Bielewski ◽  

Possibility to use Modular Total Absorption Spectrometer (MTAS) as a device to measure complete decay scheme, including β-n of neutron rich isotopes, has been investigated. Analysis of well known 87Br with its 2.6% β-n branching ratio served as a test case. Preliminary results agree with the published data.


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