Acceleration mechanisms of energetic ion debris in laser-driven tin plasma EUV sources

Author:

Totorica S. R.12ORCID,Lezhnin K.3ORCID,Hemminga D. J.45ORCID,Gonzalez J.4ORCID,Sheil J.45ORCID,Diallo A.3ORCID,Hyder A.6ORCID,Fox W.13ORCID

Affiliation:

1. Department of Astrophysical Sciences, Princeton University 1 , Princeton, New Jersey 08544, USA

2. Department of Astro-fusion Plasma Physics (AFP), Headquarters for Co-Creation Strategy, National Institutes of Natural Sciences 2 , Tokyo 105-0001, Japan

3. Princeton Plasma Physics Laboratory, Princeton University 3 , Princeton, New Jersey 08540, USA

4. Advanced Research Center for Nanolithography 4 , Science Park 106, 1098 XG Amsterdam, The Netherlands

5. Department of Physics and Astronomy, and LaserLaB, Vrije Universitiet Amsterdam 5 , De Boelelaan 1081, 1081 HV Amsterdam, The Netherlands

6. Department of Applied Physics and Applied Mathematics, Columbia University 6 , New York, New York 10027, USA

Abstract

Laser-driven tin plasmas are driving new-generation nanolithography as sources of extreme ultraviolet (EUV) radiation centered at 13.5 nm. A major challenge facing industrial EUV source development is predicting energetic ion debris produced during the plasma expansion that may damage the sensitive EUV channeling multilayer optics. Gaining a detailed understanding of the plasma dynamics and ion acceleration mechanisms in these sources could provide critical insights for designing debris mitigation strategies in future high-power EUV sources. We develop a fully kinetic model of tin-EUV sources using one-dimensional particle-in-cell simulations to study ion debris acceleration, which will be valuable for cross-validation of radiation-hydrodynamic simulations. An inverse-bremsstrahlung heating operator is used to model the interaction of a tin target with an Nd:YAG laser, and thermal conduction is included through a Monte Carlo Coulomb collision operator. While the large-scale evolution is in reasonable agreement with analogous hydrodynamic simulations, the significant timescale for collisional equilibration between electrons and ions allows for the development of prominent two-temperature features. A collimated flow of energetic ions is produced with a spectrum that is significantly enhanced at high energies compared to fluid simulations. The dominant acceleration mechanism is found to be a large-scale electric field supported mainly by the electron pressure gradient, which is enhanced in the kinetic simulations due to the increased electron temperature. We discuss the implications of these results for future modeling of tin-EUV sources and the development of debris mitigation schemes.

Funder

U.S. Department of Energy

Advanced Research Center for Nanolithography

Publisher

AIP Publishing

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