%0 Generic %1 samui2017efficient %A Samui, Saumyadip %A Subramanian, Kandaswamy %A Srianand, Raghunathan %D 2017 %K IGM cosmic ray wind %T Efficient cold outflows driven by cosmic rays in high redshift galaxies and their global effects on the IGM %U http://arxiv.org/abs/1706.01890 %X We present semi-analytical models of galactic outflows in high redshift galaxies driven by both hot thermal gas and non-thermal cosmic rays. Thermal pressure alone can not sustain a large scale outflow in low mass galaxies (i.e $M10^8$M$_ødot$), in the presence of supernovae (SNe) feedback with large mass loading. We show that inclusion of cosmic ray pressure allows outflow solutions even in these galaxies. In massive galaxies for the same energy efficiency, cosmic ray winds can propagate to larger distances compared to pure thermally driven winds. On an average gas in the cosmic ray driven winds has a lower temperature and detecting it through absorption lines becomes easier. Using our constrained semi-analytical models of galaxy formation (that explains the observed UV luminosity functions of galaxies) we study the influence of cosmic ray driven winds on the properties of the inter galactic medium (IGM) at different redshifts. In particular, we study the volume filling factor, average metallicity, cosmic ray and magnetic field energy density for models invoking atomic cooled and molecular cooled halos. We show that the residual cosmic rays could have enough energy that can be transferred to the thermal gas in presence of magnetic fields to influence the thermal history of the intergalactic medium. The significant volume filling and resulting strength of IGM magnetic fields can also account for recent $\gamma$-ray observations of blazars.

@misc{samui2017efficient, abstract = {We present semi-analytical models of galactic outflows in high redshift galaxies driven by both hot thermal gas and non-thermal cosmic rays. Thermal pressure alone can not sustain a large scale outflow in low mass galaxies (i.e $M\sim 10^8$M$_\odot$), in the presence of supernovae (SNe) feedback with large mass loading. We show that inclusion of cosmic ray pressure allows outflow solutions even in these galaxies. In massive galaxies for the same energy efficiency, cosmic ray winds can propagate to larger distances compared to pure thermally driven winds. On an average gas in the cosmic ray driven winds has a lower temperature and detecting it through absorption lines becomes easier. Using our constrained semi-analytical models of galaxy formation (that explains the observed UV luminosity functions of galaxies) we study the influence of cosmic ray driven winds on the properties of the inter galactic medium (IGM) at different redshifts. In particular, we study the volume filling factor, average metallicity, cosmic ray and magnetic field energy density for models invoking atomic cooled and molecular cooled halos. We show that the residual cosmic rays could have enough energy that can be transferred to the thermal gas in presence of magnetic fields to influence the thermal history of the intergalactic medium. The significant volume filling and resulting strength of IGM magnetic fields can also account for recent $\gamma$-ray observations of blazars.}, added-at = {2017-06-08T09:53:54.000+0200}, author = {Samui, Saumyadip and Subramanian, Kandaswamy and Srianand, Raghunathan}, biburl = {https://www.bibsonomy.org/bibtex/2451ff6484fccf6241b5a43535d23e7c1/miki}, description = {[1706.01890] Efficient cold outflows driven by cosmic rays in high redshift galaxies and their global effects on the IGM}, interhash = {9ffd440ad05e2a917ce0ea72ed2a83b5}, intrahash = {451ff6484fccf6241b5a43535d23e7c1}, keywords = {IGM cosmic ray wind}, note = {cite arxiv:1706.01890Comment: 15 Pages, 9 figures, Submitted to MNRAS}, timestamp = {2017-06-08T09:53:54.000+0200}, title = {Efficient cold outflows driven by cosmic rays in high redshift galaxies and their global effects on the IGM}, url = {http://arxiv.org/abs/1706.01890}, year = 2017 }