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The energy and the angular dependence of the associative vector charmed${D^*}$-meson photoproduction, $\gamma+N\to {\cal B}_c+ \overline{D^*}$, with${\cal B}_c=\Lambda_c$ or $\Sigma_c$, has been predicted in framework ofpseudoscalar D-meson exchange model. The behavior of the cross section isdriven by phenomenological form factors, which can be parametrized in terms oftwo independent parameters. The predicted values of the cross section aresizeable enough to be measured in the near threshold region.Comment: 10 pages 4 figure

physical review. d. particles, fields, gravitation, and cosmology/physical review. d. particles and fields

Photoproduction of charmed vector mesons,<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>γ</mml:mi><mml:mo>+</mml:mo><mml:mrow><mml:mrow><mml:mover><mml:mrow><mml:mi>N</mml:mi></mml:mrow><mml:mrow><mml:mo>→</mml:mo></mml:mrow></mml:mover></mml:mrow></mml:mrow><mml:mrow><mml:msub><mml:mrow><mml:mi mathvariant="script">B</mml:mi></mml:mrow><mml:mrow><mml:mi>c</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mo>+</mml:mo><mml:mrow><mml:mrow><mml:mover><mml:mrow><mml:…

Photoproduction of charmed vector mesons,γ+N→Bc+