Maximum brightness temperature of an incoherent synchrotron source: Inverse compton limit - A misnomer

Abstract

We show that an upper limit of ∼1012 K on the peak brightness temperature for an incoherent synchrotron radio source, commonly referred to in the literature as an inverse Compton limit, really may not be due to inverse Compton effects. We show that a somewhat tighter limit T eq ∼ 1011 is actually obtained for the condition of equipartition of energy between radiating particles and magnetic fields, which happens to be a configuration of minimum energy for a self-absorbed synchrotron radio source. An order of magnitude change in brightness temperature from T eq in either direction would require departures from equipartition of about 8 orders of magnitude, implying a change in total energy of the system up to ∼104 times the equipartition value. Constraints of such extreme energy variations imply that brightness temperatures may not depart much from T eq. This is supported by the fact that at the spectral turnover, brightness temperatures much lower than ∼1011 K are also not seen in VLBI observations. Higher brightness temperatures in particular would require in the source not only many orders of magnitude higher additional energy for the relativistic particles but also many orders of magnitude weaker magnetic fields. Diamagnetic effects do not allow such extreme conditions, keeping the brightness temperatures close to the equipartition value, which is well below the limit where inverse Compton effects become important. © 2009. The American Astronomical Society.