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We present polarization-sensitive images from the Karl G. Jansky Very LargeArray (VLA) at 5 GHz of 11 radio-quiet PG quasars. Based on the radiomorphology, spectral index and polarization properties from the VLA study,coupled with the findings of our previous 685 MHz uGMRT data, we find thepresence of low-powered jets on sub-arcsecond and arcsecond scales in 9sources; some show signatures of bent jets. The origin of radio emissionremains unclear in the remaining 2 sources. Of the 11 sources, linearpolarization is detected in four of them with fractional polarization rangingbetween 2% and 25%. In PG 1229+204, the inferred B-field direction is parallelto the local kpc-scale jet direction. The inferred B-fields are transverse tothe weak southward extension in PG 0934+013. For PG 0050+124 and PG 0923+129,the relationship between the B-field structure and radio outflow directionremains unclear. Localized or small-scale jet-medium interactions can beinferred across the sample based on the VLA jet kinetic power arguments andpolarization data. These may have the potential as a feedback mechanism. Wefind that the radio properties do not show strong correlations with the starformation, [O~III] and CO quantities published in the literature. The lack ofevidence of AGN feedback on the global galaxy properties could be due to therelative time scales of AGN activity and those over which any impact might betaking place.

Probing the interplay between jets, winds and multi-phase gas in 11 radio-quiet PG Quasars: A uGMRT-VLA study