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Multiplicity of Secondary Particles in Inelastic Proton - Neon Interactions at 300-{GeV}/$c$

Azimov, S.A. ; Inogamov, Sh.V. ; Kosonovsky, E.A. ; et al.
Phys.Rev.D 23 (1981) 2512, 1981.
Inspire Record 10318 DOI 10.17182/hepdata.17871

The data on the total inelastic and partial cross sections in pNe interactions at 300 GeV are presented. It is found that the total cross section, σin(pNe)=356±13 mb, and multiplicity distributions of the number of negative and relativistic charged particles are in good agreement with predictions of a multiple-scattering model based on Glauber's approach. The multiplicity of negative particles obeys the Koba-Nielsen-Olesen (KNO) scaling, but it is observed that the KNO function depends on the atomic mass number of the target. From an analysis of the average multiplicities of secondary particles, it is shown that approximately 10 percent of the fast (p≳1.2 GeV) positive secondaries are protons, which are derived from the nucleons in the neon nucleus.

13 data tables
Table 1

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Nuclear absorption cross-sections for pions, kaons, protons, and anti-protons in the momentum range 6-60 gev/c

Gorin, Yu.P. ; Denisov, S.P. ; Donskov, S.V. ; et al.
Yad.Fiz. 18 (1973) 336-347, 1973.
Inspire Record 84864 DOI 10.17182/hepdata.18400
10 data tables
Table 1

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ANTI-PROTON INTERACTION CROSS-SECTIONS WITH C, AL, TI, AND CD NUCLEI IN THE REGION OF 1.5-GEV/C. (IN RUSSIAN)

Afonasev, V.N. ; Borisov, V.S. ; Borodina, I.N. ; et al.
Yad.Fiz. 40 (1984) 34-42, 1984.
Inspire Record 215359 DOI 10.17182/hepdata.2554

None

4 data tables
Table 1

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Inelastic cross-sections and multiplicities of secondary charged particles produced in collisions of relativistic nuclei with carbon and tantalum at 2.3-A-GeV/c and 4.2-A-GeV/c

Grigalashvili, N.S. ; Kutsidi, N.K. ; Tevzadze, Yu.V. ; et al.
Sov.J.Nucl.Phys. 48 (1988) 301-305, 1988.
Inspire Record 457969 DOI 10.17182/hepdata.17347

None

20 data tables
Table 1

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The interaction cross-section of protons with nuclei of air atoms at energies 2 x 10**16-eV

Efimov, N.N. ; Zhukov, V.Yu. ; Kalmykov, N.N. ; et al.
Sov.J.Nucl.Phys. 49 (1989) 558-559, 1989.
Inspire Record 292948 DOI 10.17182/hepdata.17328

None

1 data table
Table 1

NUCLEUS IS AVERAGE AIR NUCLEUS.


DETERMINATION OF CROSS-SECTIONS OF INELASTIC INTERACTION OF PIONS AND NUCLEONS WITH FE NUCLEI IN THE ENERGY INTERVAL 0.5-TEV - 5-TEV. (IN RUSSIAN)

Avakian, V.V. ; Garyaka, A.P. ; Gevorkian, S.R. ; et al.
Yad.Fiz. 40 (1984) 949-959, 1984.
Inspire Record 218762 DOI 10.17182/hepdata.17632

None

4 data tables
Table 1

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DETERMINING INELASTIC INTERACTION CROSS-SECTIONS FOR NUCLEONS AND PIONS INCIDENT ON CARBON AND LEAD NUCLEI AT 0.5-TEV - 5-TEV

Avakian, V.V. ; Gevorkian, S.P. ; Zhamkochian, V.M. ; et al.
Bull.Russ.Acad.Sci.Phys. 50N11 (1986) 4-7, 1986.
Inspire Record 242221 DOI 10.17182/hepdata.41509

None

1 data table
Table 1

No description provided.


Inelastic cross-section for p-air collisions from air shower experiment and total cross-section for p p collisions at SSC energy

Honda, M. ; Nagano, M. ; Tonwar, S. ; et al.
Phys.Rev.Lett. 70 (1993) 525-528, 1993.
Inspire Record 342678 DOI 10.17182/hepdata.19743

Based on an analysis of the extensive air shower data accumulated over the last ten years at Akeno Cosmic Ray Observatory, the value of the proton-air nuclei inelastic cross section (σinp−air) has been determined assuming the validity of quasi-Feynman scaling of particle production in the fragmentation region. The energy dependence of σinp−air can be represented as 290(E/1 TeV)0.052 mb in the energy interval 1016.2–1017.6 eV, where E is the incident proton energy. The total p-p cross section (σtotp−p), derived using the nuclear distribution function obtained from the shell model, increases with energy as 38.5+1.37 ln2(√s /10 GeV) mb.

2 data tables
Table 1

No description provided.

Table 2

Best fit to data gives SIG(PP) = 38.5 + 1.37*LN(SQRT(S)/10 GeV)**2.


Scaling of the multiplicity in hadron nucleus interactions

Adamovic, O. ; Drndarevic, S. ; Krpic, D. ; et al.
Phys.Rev.C 48 (1993) 2772-2774, 1993.
Inspire Record 366047 DOI 10.17182/hepdata.26003

It is shown that in interactions of protons at 200, 300, and 400 GeV, and negative pions at 300 GeV with emulsion nuclei, the scaling of the multiplicity of relativistic charged secondaries is valid and described by a linear function of the scaling variable, z.

2 data tables
Table 1

No description provided.

Table 2

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Longitudinal evolution of extensive air showers according to the results of Cherenkov light studies

Kalmykov, N.N. ; Khristiansen, G.B. ; Prosin, V.V. ;
Phys.Atom.Nucl. 58 (1995) 1563-1568, 1995.
Inspire Record 407049 DOI 10.17182/hepdata.17206

None

1 data table
Table 1

NUCLEUS is air nucleus.