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Production of neutrons in Pb, Cd, Fe, and Al under the influence of cosmic-ray muons at a depth of 150 m water equivalent

Gorshkov, G.V. ; Zyabkin, V.A. ;
Sov.J.Nucl.Phys. 7 (1968) 470-474, 1968.
Inspire Record 1392567 DOI 10.17182/hepdata.17076

None

1 data table
Table 1

No description provided.


Search for neutrino emission from relic dark matter in the Sun with the Baikal NT200 detector

The Baikal collaboration Avrorin, A.D. ; Avrorin, A.V. ; Aynutdinov, V.M. ; et al.
Astropart.Phys. 62 (2015) 12-20, 2015.
Inspire Record 1296058 DOI 10.17182/hepdata.64126

We have analyzed a data set taken over 2.76 years live time with the Baikal neutrino telescope NT200. The goal of the analysis is to search for neutrinos from dark matter annihilation in the center of the Sun. Apart from the conventional annihilation channels $b\bar{b}$, $W^+W^-$ and $\tau^+\tau^-$ we consider also the annihilation of dark matter particles into monochromatic neutrinos. From the absence of any excess of events from the direction of the Sun over the expected background, we derive 90% upper limits on the fluxes of muons and muon neutrinos from the Sun, as well as on the elastic cross sections of dark matter scattering on protons.

6 data tables
Table 1

Process: DM DM --> BOTTOM BOTTOMBAR. Half-cone angle GAMMA, 90% upper limit N(SIGNAL) on the number of signal events, the muon flux PHI(MU), the dark matter annihilation rate in the Sun GAMMA(ANN), the dark matter-proton spin-dependent SIG(SD) and spin-independent SIG(SI) scattering cross sections and neutrino flux PHI(NU).

Table 2

Process: DM DM --> TAU+ TAU-. Half-cone angle GAMMA, 90% upper limit N(SIGNAL) on the number of signal events, the muon flux PHI(MU), the dark matter annihilation rate in the Sun GAMMA(ANN), the dark matter-proton spin-dependent SIG(SD) and spin-independent SIG(SI) scattering cross sections and neutrino flux PHI(NU).

Table 3

Process: DM DM --> W+ W-. Half-cone angle GAMMA, 90% upper limit N(SIGNAL) on the number of signal events, the muon flux PHI(MU), the dark matter annihilation rate in the Sun GAMMA(ANN), the dark matter-proton spin-dependent SIG(SD) and spin-independent SIG(SI) scattering cross sections and neutrino flux PHI(NU).

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Anti-proton helium-3 annihilation at 55-MeV/c

Bianconi, A. ; Bonomi, G. ; Bussa, M.P. ; et al.
Phys.Lett.B 492 (2000) 254-258, 2000.
Inspire Record 538722 DOI 10.17182/hepdata.27999

The p̄ 3 He annihilation cross section is measured for the first time in the momentum interval (50÷60) MeV/ c . About 9000 pictures collected by the Streamer Chamber Collaboration (PS179) at LEAR–CERN have been scanned. Six events are found, corresponding to σ ann =1850±700 mb. The result is compared to the set of measurements presently available in the region of low p̄ momentum.

1 data table
Table 1

The mean beam momentum at the center of the fiducial volume = 55 MeV.


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.


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.