  Only four globular cluster planetary nebulae (GCPN) are known so far in the
Milky Way. About 50 new globular clusters have been recently discovered towards
the Galactic bulge. We present a search for planetary nebulae within 3 arcmin
of the new globular clusters, revealing the identification of new candidate
GCPN. These possible associations are PN SB 2 with the GC Minni 06, PN
G354.9-02.8 with the GC Minni 11, PN G356.8-03.6 with the GC Minni 28, and PN
Pe 2-11 with the GC Minni 31. We discard PN H 2-14 located well within the
projected tidal radius of the new globular cluster FSR1758 because they have
different measured radial velocities. These are interesting objects that need
follow-up observations (especially radial velocities) in order to confirm
membership, and to measure their physical properties in detail. If confirmed,
this would double the total number of Galactic GCPN.
