Scalar Bremsstrahlung in Gravity-Mediated Ultrarelativistic Collisions

Classical bremsstrahlung of a massless scalar field $Φ$ is studied in gravity mediated ultra-relativistic collisions with impact parameter $b$ of two massive point particles in the presence of $d$ non-compact or toroidal extra dimensions. The spectral and angular distribution of the scalar radiation are analyzed, while the total emitted $Φ-$energy is found to be strongly enhanced by a $d-$dependent power of the Lorentz factor $γ$. The direct radiation amplitude from the accelerated particles is shown to interfere destructively (in the first two leading ultra-relativistic orders) with the one due to the $Φ-Φ-graviton$ interaction in the frequency regime $γ/b\lesssim ω\lesssim γ^2/b$ in all dimensions.

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