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Measurements of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>π</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi>η</mml:mi></mml:mrow><mml:mrow><mml:mn>0</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>Photoproduction at Incident Gamma-Ray Energies of 6.0-17.8 GeV

Richard I. AndersonStanford Linear Accelerator Center, Stanford, CaliforniaD.B. GustavsonStanford Linear Accelerator Center, Stanford, CaliforniaJ. R. JohnsonStanford Linear Accelerator Center, Stanford, CaliforniaD. M. RitsonStanford Linear Accelerator Center, Stanford, CaliforniaW.G. JonesStanford Linear Accelerator Center, Stanford, CaliforniaD. L. KreinickStanford Linear Accelerator Center, Stanford, CaliforniaF. V. MurphyStanford Linear Accelerator Center, Stanford, CaliforniaR. WeinsteinStanford Linear Accelerator Center, Stanford, California
1968lv
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We report on cross-sectional measurements on the photoproduction of ${\ensuremath{\pi}}^{0}$ and ${\ensuremath{\eta}}^{0}$ mesons on hydrogen for a range in $t$ of -0.2 to -0.9 ${(\mathrm{G}\mathrm{e}\mathrm{V}/\mathit{c})}^{2}$ and for a range of energies 6.0-16.0 GeV. The sharp dip observed at lower energies at $t=\ensuremath{-}0.5$ for ${\ensuremath{\pi}}^{0}$ production becomes less pronounced at higher energies. This implies in the Regge framework the ${B}^{0}$ meson trajectory dominates at higher energies. Our one angular distribution for ${\ensuremath{\eta}}^{0}$ production at 6.0 GeV shows no dip at $t=\ensuremath{-}0.5$ as do the ${\ensuremath{\pi}}^{0}$ data.

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