We calculated the solar monopole abundance limit by comparing the observed solar neutrino flux and the calculation of non-fusion solar neutrino flux produced by Rubakov process in the solar core. We included the produced meson's enhancement effects by the surrounding ions in the solar core. We find that the monopole number N M < 1.9 × 10 20 ( 1 m b / σ 0 ) , where σ 0 is the characteristic proton decay cross section of Rubakov process. This is similar or stronger than strong limits obtained from neutron star's luminosity.

• LEE HAESHIM(Department of Physics, Chungnam National University)
• LEE HOYUN(Department of Physics, Chungnam National University)
• KOH YOON SUK(Department of Physics, Wonkwnag University)