Search for neutrino interactions with the MAC-1

Aleshin, Yu.D. ; Egorov, O.K. ; Kolganova, E.D. ; et al.
ITEP-23-96, 1996.
Inspire Record 422193 DOI 10.17182/hepdata.39974

None

1 data table

No description provided.


Mean multiplicities of the final hadron states in neutrino nuclear interactions at E(nu) = 8.7-GeV

Aleshin, Yu.D. ; Egorov, O.K. ; Smirnitsky, V.A. ; et al.
J.Exp.Theor.Phys. 83 (1996) 208-209, 1996.
Inspire Record 431676 DOI 10.17182/hepdata.17007

None

1 data table

No description provided.


Inclusive characteristics of neutrino scattering at the nuclei of a photographic emulsion at energies of E(nu) = 3-GeV - 30-GeV

Aleshin, Yu.D. ; Egorov, O.K. ; Smirnitsky, V.A. ; et al.
J.Exp.Theor.Phys. 83 (1996) 205-207, 1996.
Inspire Record 431675 DOI 10.17182/hepdata.17061

None

1 data table

No description provided.


Fragmentation characteristics of relativistic carbon nucleus at its interaction with hydrogen

Belaga, V.V. ; Bondarenko, A.I. ; Karshiev, D.A. ; et al.
Phys.Atom.Nucl. 59 (1996) 991-996, 1996.
Inspire Record 404821 DOI 10.17182/hepdata.38625

None

3 data tables

FRAGB - BEAM FRAGMENT WITH Z>=2.


Fragmentation of relativistic carbon nuclei undergoing inelastic collisions with progane and tantalum nuclei.

Belaga, V.V. ; Bondarenko, A.I. ; Kanarek, T. ; et al.
Phys.Atom.Nucl. 59 (1996) 1935-1941, 1996.
Inspire Record 403063 DOI 10.17182/hepdata.17175

None

8 data tables

C3H8 nucleus. P, DEUT and TRITIUM in the final state are considered as spectators.

P, DEUT and TRITIUM in the final state are considered as spectators.

C_3 H_8 nucleus. P in the final state are considered as spectators.

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Study of D*+ and search for D**0 production by neutrinos in BEBC

The Big Bubble Chamber Neutrino collaboration Asratvan, A.E. ; Aderholz, M. ; Ammosov, V.V. ; et al.
Z.Phys.C 68 (1995) 43-46, 1995.
Inspire Record 395454 DOI 10.17182/hepdata.47928

Data from BEBC experiments are combined to provide large statistics for neutrino interactions. ChargedD* mesons are produced in (1.22±0.25)% of neutrino and (1.01±0.31)% of antineutrino charged current interactions. The mean fraction of the hadronic laboratory energy taken by theD*+ in these events is 0.59±0.03±0.08. Less than 18% of all chargedD* mesons from (anti)neutrino interactions are found to be daughters ofD**0 (at the 90% confidence level).

4 data tables

Mean fractional hadronic energy carried by the D*+- in the laboratory system.

Mean value of the Bjorken scaling variable X.

Rate of charged D* meson production per charged current neutrino interaction.

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Total cross-section measurements for muon-neutrino, anti-muon-neutrino interactions in 3-GeV - 30-GeV energy range with IHEP-JINR neutrino detector

Anikeev, V.B. ; Belikov, S.V. ; Borisov, A.A. ; et al.
Z.Phys.C 70 (1996) 39-46, 1996.
Inspire Record 400486 DOI 10.17182/hepdata.40711

The results of total cross section measurements for theνμ,\(\bar \nu _\mu\) interactions with isoscalar target in the 3 – 30 GeV energy range have been presented. The data were obtained with the IHEP-JINR Neutrino Detector in the “natural” neutrino beams of the U-70 accelerator. Neutrino fluxes were obtained by averaging the spectra, based on the calculations with the use of the experimental data on secondary particle yields from the target and muon fluxes measurements in 9 gaps of the muon filter, as well as the spectra determined from quasi-elastic events and spectra defined by extrapolating differential distributiondσ/dy in the regiony=0. The significant deviation from the linear dependence forσtot versus neutrino energy is determined in the energy range less than 15 GeV.

2 data tables

No description provided.

No description provided.


On slow-particle production in 200-A-GeV O-16 emulsion interactions

El-Nadi, M. ; Sherif, M.M. ; Hussien, A. ; et al.
Nuovo Cim.A 108 (1995) 87-96, 1995.
Inspire Record 408539 DOI 10.17182/hepdata.37839

The multiplicity distributions and the correlations of different types of slow particles produced in 200A GeV oxygen-induced interactions with emulsion nuclei are presented. The experimental distributions are studied within the framework of the generalized Andersson-Otterlund-Stenlund (AOS) model for nucleus-nucleus interactions. The generalized (AOS) model fails to describe the present experimental data. Also a systematic comparison using the calculations of VENUS model is made. The grey-particles multiplicity is successfully reproduced by the theoretical multistring model VENUS, while the model is inadequate for explaining the distribution of black particles.

1 data table

No description provided.


Rescattering probed by the emission of slow target associated particles in high-energy heavy ion interactions

The EMU01 collaboration Adamovich, M.I ; Aggarwal, M.M ; Alexandrov, Y.A ; et al.
Phys.Lett.B 363 (1995) 230-236, 1995.
Inspire Record 406952 DOI 10.17182/hepdata.28438

In this letter the distribution of slow target associated particles emitted in Au + Emulsion interactions at 11.6 A GeV/ c is studied. The three models RQMD, FRITIOF and VENUS are used for comparisons and especially their treatment of rescattering is investigated.

6 data tables

No description provided.

PROJECTILE ASSOCIATED HE-FRAGMENTS.

No description provided.

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Nuclear structure function in carbon near x = 1

The BCDMS collaboration Benvenuti, A.C. ; Bollini, D. ; Camporesi, T. ; et al.
Z.Phys.C 63 (1994) 29-36, 1994.
Inspire Record 374300 DOI 10.17182/hepdata.48235

Data from deep inelastic scattering of 200 GeV muons on a carbon target with squared four-momentum transfer 52 GeV2≤Q2≤200 GeV2 were analysed in the region of the Bjorken variable close tox=1, which is the kinematic limit for scattering on a free nucleon. At this value ofx, the carbon structure function is found to beF2C≈1.2·10−4. Thex dependence of the structure function forx>0.8 is well described by an exponentialF2C∞exp(−sx) withs=16.5±0.6.

5 data tables

No description provided.

Multiplicative factors by which F2 has to be multiplied or divided to allow for a systematic uncertainty in detector resolution.

Multiplicative factors by which F2 has to be multiplied or divided to allow for a systematic uncertainty in the beam energy.

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