BH Mass, Jet and Accretion Disk Connection: An Analysis of Radio-loud
  and Radio-quiet Quasars
  Surveys have shown radio-loud (RL) quasars constitute $10 \%$-$15 \%$ of the
total quasar population. However, it is unknown if the radio-loud fraction (RL
quasars/Total quasars) remains consistent among different parameter spaces.
This study shows that radio-loud fraction increases for increasing full width
half maximum (FWHM) velocity of the H$\beta$ and MgII broad emission line. Our
data has been obtained from Shen et al. (2011) catalogue. To investigate the
reason, in this preliminary study we analyse various properties like bolometric
luminosity, optical continuum luminosity, black hole (BH) mass and accretion
rate of RL quasars and RQ quasars sample which have FWHM greater than 15000km/s
(High broad line). From the distributions we can conclude for all the
properties in high broad line, RL quasars are having higher values than RQ
quasars. We have predicted RL quasars are intrinsically brighter than RQ
quasars and also predicted BH mass-jet connection and accretion disk-jet
connection from our results but to conclude anything more analysis is needed.
