Electron Weibel instability induced magnetic fields in optical-field ionized plasmas

Author:

Zhang Chaojie1ORCID,Wu Yipeng1ORCID,Sinclair Mitchell1,Farrell Audrey1,Marsh Kenneth A.1,Hua Jianfei2ORCID,Petrushina Irina3ORCID,Vafaei-Najafabadi Navid3ORCID,Kupfer Rotem4ORCID,Kusche Karl4ORCID,Fedurin Mikhail4,Pogorelsky Igor4ORCID,Polyanskiy Mikhail4ORCID,Huang Chen-Kang5ORCID,Lu Wei2,Mori Warren B.16ORCID,Joshi Chan1ORCID

Affiliation:

1. Department of Electrical and Computer Engineering, University of California Los Angeles, Los Angeles, 90095 California, USA

2. Department of Engineering Physics, Tsinghua University, 100084 Beijing, China

3. Department of Physics and Astronomy, Stony Brook University, Stony Brook, 11794 New York, USA

4. Accelerator Test Facility, Brookhaven National Laboratory, Upton, 11973 New York, USA

5. Institute of Atomic and Molecular Sciences, Academia Sinica, 10617 Taipei, Taiwan

6. Department of Physics and Astronomy, University of California Los Angeles, Los Angeles, 90095 California, USA

Abstract

Generation and amplification of magnetic fields in plasmas is a long-standing topic that is of great interest to both plasma and space physics. The electron Weibel instability is a well-known mechanism responsible for self-generating magnetic fields in plasmas with temperature anisotropy and has been extensively investigated in both theory and simulations, yet experimental verification of this instability has been challenging. Recently, we demonstrated a new experimental platform that enables controlled initialization of highly nonthermal and/or anisotropic plasma electron velocity distributions via optical-field ionization. Using an external electron probe bunch from a linear accelerator, the onset, saturation, and decay of the self-generated magnetic fields due to electron Weibel instability were measured for the first time to our knowledge. In this paper, we will first present experimental results on time-resolved measurements of the Weibel magnetic fields in non-relativistic plasmas produced by Ti:Sapphire laser pulses (0.8  μm) and then discuss the feasibility of extending the study to a quasi-relativistic regime by using intense CO2 (e.g., 9.2  μm) lasers to produce much hotter plasmas.

Funder

Office of Naval Research

Air Force Office of Scientific Research

U.S. Department of Energy

National Science Foundation

National Natural Science Foundation of China

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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