Shopping cart


Rachel Rosen (Columbia University)

Date: Tue. November 8th, 2016, 11:00 am-12:00 pm
Location: Miller room

Non-Singular Black Holes in Massive Gravity

When starting with a static, spherically-symmetric ansatz, there are currently two types of black hole solutions in massive gravity: (i) exact Schwarzschild solutions which exhibit no Yukawa suppression at large distances and (ii) solutions which contain coordinate-invariant singularities at the horizon.  In this talk, I will present new black hole solutions which have a nonsingular horizon and can potentially be matched to Yukawa asymptotics at large distances.  These solutions recover Schwarzschild black holes in the massless limit and are thus observationally viable.”

Scroll To Top