Scalar bremsstrahlung in gravity-mediated ultrarelativistic collisions. (English) Zbl 1306.81309
Summary: Classical bremsstrahlung of a massless scalar field {\(\Phi\)} 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 {\(\Phi\)}-energy is found to be strongly enhanced by a \(d\)-dependent power of the Lorentz factor \(\gamma\). 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 {\(\Phi\)}-{\(\Phi\)}-\(graviton\) interaction in the frequency regime \( \gamma /b \lesssim \omega \lesssim {\gamma^2}/b \) in all dimensions.
MSC:
| 81U05 | \(2\)-body potential quantum scattering theory |
| 83E15 | Kaluza-Klein and other higher-dimensional theories |
| 83C57 | Black holes |
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