Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session TO8: Plasma Acceleration: Computation, Beam Driven, Mid-IR lasers
9:30 AM–12:30 PM,
Thursday, November 8, 2018
OCC
Room: C120-122
Chair: Jessica Shaw, Laboratory for Laser Energetics, Rochester, NY
Abstract ID: BAPS.2018.DPP.TO8.12
Abstract: TO8.00012 : Observation of arrest of Kerr self-focusing in a 10 μm filament in air at 1 TW/cm2 clamped intensity*
11:42 AM–11:54 AM
Presenter:
Sergei Tochitsky
(UCLA)
Authors:
Sergei Tochitsky
(UCLA)
Eric Welch
(UCLA)
Mikhail Polyanskiy
(BNL)
Igor Pogorelsky
(BNL)
Paris Panagiotopoulos
(University of Arizona)
Miroslav Kolesik
(University of Arizona)
Ewan M Wright
(University of Arizona)
Stephan W Koch
(University of Arizona)
Jerome V Moloney
(University of Arizona)
Jeremy Pigeon
(UCLA)
Chan Joshi
(UCLA)
In this paper we demonstrate for the first time self-guiding of a 10.2 μm ~1TW CO2 laser pulse in the atmosphere over at least 30 meters (~20 ZR). We observe that when the peak power of such pulses exceeds ~870 GW, a centimeter-diameter single filament is formed in air. We call such a single filament a megafilament because it confines an ~1TW laser pulse with several Joules of energy and its cross-section is 104 times larger than a typical near-IR single filament. The clamped intensity of ~1 TW/cm2 for the long-wave infrared light confined in this megafilament was measured to be much smaller than that required for the tunnel ionization of O2/N2. By anchoring the experimental data with numerical simulations based on the concept of many-body interactions in the atmospheric pressure gas, we find that Kerr self-focusing at such a low laser intensity is arrested by a new and different ionization mechanism due to many-body Coulomb ionization . The amount of free carriers produced inside of the filament is rather small (≤1013cm-3) but sufficient to effectively decrease the molecular polarizability during the laser pulse.
*This material is based on work supported by the AFOSR under award number FA9550-16-1-0139 DEF and the ONR MURI (4-442521- JC-22891).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.TO8.12
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2024 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700