Photoproduction
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pi0 and rho0 Photoproduction from 6-GeV to 18-GeV

Barish, B. ; Gomez, R. ; Kreinick, D. ; et al.
Phys.Rev.D 9 (1974) 566, 1974.
Inspire Record 94529 DOI 10.17182/hepdata.21952

Differential cross sections for π0 and ρ0 photoproduction from protons have been measured at photon energies 6, 12, and 18 GeV and momentum transfers 0.5 to 3 (GeVc)2.

3 data tables
Table 1

No description provided.

Table 2

No description provided.

Table 3

No description provided.


pi0 photoproduction on the proton for photon energies from 0.675-GeV to 2.875-GeV.

Dugger, M. ; Ritchie, Barry G. ; Ball, J.P. ; et al.
Phys.Rev.C 76 (2007) 025211, 2007.
Inspire Record 749989 DOI 10.17182/hepdata.51855

Differential cross sections for the reaction $\gamma p \to p \pi^0$ have been measured with the CEBAF Large Acceptance Spectrometer (CLAS) and a tagged photon beam with energies from 0.675 to 2.875 GeV. The results reported here possess greater accuracy in the absolute normalization than previous measurements. They disagree with recent CB-ELSA measurements for the process at forward scattering angles. Agreement with the SAID and MAID fits is found below 1 GeV. The present set of cross sections has been incorporated into the SAID database, and exploratory fits have been extended to 3 GeV. Resonance couplings have been extracted and compared to previous determinations.

45 data tables
Table 1

Differential cross section for indicent photon energy 675 MeV.

Table 2

Differential cross section for indicent photon energy 725 MeV.

Table 3

Differential cross section for indicent photon energy 775 MeV.

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η photoproduction cross-section for incident photon energies from 800 to 1000 MeV

Bacci, C. ; Penso, G. ; Salvini, G. ; et al.
Nuovo Cim.A 45 (1966) 983-1009, 1966.
Inspire Record 1185323 DOI 10.17182/hepdata.37560

Photoproduction cross-section of the η-particle for incident photon energiesK from ∼800 to ∼1000 MeV has been measured at the 1.1 GeV Frascati electronsynchrotron. The differential cross-section for this process, at a c.m. angle of the η of ∼110°, turns out to be fairly constant for 830 MeV≤K≤900 MeV, and drops down by a factor 5 to 10 atK=950 MeV. These results are discussed in terms of a comparison with the data on the production of η's by pions, and with the data on pion-nucleon scattering and pion photoproduction. The conclusions are in agreement with the hypothesis that the η-N system is dominated at low energies by a resonance with orbital angular momentuml=0 (S 1/2,1/2 resonance).

1 data table
Table 1

No description provided.