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Using the Polyakov--Nambu--Jona-Lasinio model the strange quark chiral phasetransition and the effect of its current mass on a hot magnetized three flavorquark matter at zero chemical potential is investigated. The impact of the 'tHooft mixing term on the restoration of the chiral symmetry on the light andstrange sectors is studied and the critical temperature dependence on themagnetic field strength of the chiral strange transition is analyzed. It isshown that the s quark is much less sensitive to the magnetic field than thelight quarks. Due to the 't Hooft term, it has a strong influence on the lightquarks at all temperatures for small magnetic fields and for temperatures closeto the transition temperature at zero magnetic field and above for strongmagnetic fields. In particular, the large mass of the s quark makes the chiraltransition of the light sector smoother and shifted to larger temperatures. Ascalar coupling that weakens when the magnetic field increases will originatean inverse magnetic catalysis also in the s quark and smoothen the signature ofthe crossover on thermodynamical quantities such as the sound velocities or thespecific heat.

Strange quark chiral phase transition in hot 2+1-flavor magnetized quark matter