Laboratory modeling of jets from young stars using plasma focus facilities

TL;DR

This paper reviews how laboratory plasma focus experiments can model jets from young stars, providing insights into their formation and stability by replicating key physical properties observed in astrophysical jets.

Contribution

It demonstrates the feasibility of using plasma focus facilities to simulate and study astrophysical jets, bridging laboratory experiments with stellar phenomena.

Findings

Laboratory jets exhibit properties similar to young star jets.

Experimental results support theories of jet formation and stability.

Laboratory modeling offers a new approach to astrophysical research.

Abstract

Jets from young stars are used as an example to review how laboratory modeling enables advancement in understanding the main physical processes responsible for the formation and stability of these amazing objects. The discussion focuses on the options for modeling jet emissions in a laboratory experiment at the PF-3 facility at the National Research Center Kurchatov Institute. Many properties of the flows obtained using this experimental setup are consistent with the main features of jets from young stars.