Scientific Results

Laboratory measurements of resistivity in warm dense plasmas relevant to the microphysics of brown dwarfs

Year: 2015

Authors: Booth N., Robinson A.P.L., Hakel P., Clarke R.J., Dance R.J., Doria D., Gizzi LA., Gregori G., Koester P., Labate L., Levato T., Li B., Makita M., Mancini R.C., Pasley J., Rajeev P.P., Riley D., Wagenaars E., Waugh J.N., Woolsey N.C., Woolsey N.C.

Autors Affiliation: Central Laser Facility, STFC Rutherford Appleton Laboratory, Didcot OX11 0QX, UK; Department of Physics, College of Science, University of Nevada, Reno, Nevada 89557-0208, USA; Department of Physics, York Plasma Institute, University of York, Heslington York YO10 5DD, UK; School of Mathematics and Physics, Queen’s University Belfast, Belfast BT1 4NN, UK; Intense Laser Irradiation Laboratory, Istituto Nazionale di Ottica, Area della Ricerca del CNR, 56124 Pisa, Italy; Department of Physics, University of Oxford, Oxford OX4 3PU, UK

Abstract: Since the observation of the first brown dwarf in 1995, numerous studies have led to a better understanding of the structures of these objects. Here we present a method for studying material resistivity in warm dense plasmas in the laboratory, which we relate to the microphysics of brown dwarfs through viscosity and electron collisions. Here we use X-ray polarimetry to determine the resistivity of a sulphur-doped plastic target heated to Brown Dwarf conditions by an ultra-intense laser. The resistivity is determined by matching the plasma physics model to the atomic physics calculations of the measured large, positive, polarization. The inferred resistivity is larger than predicted using standard resistivity models, suggesting that these commonly used models will not adequately describe the resistivity of warm dense plasma related to the viscosity of brown dwarfs.

Journal/Review: NATURE COMMUNICATIONS

Volume: 6      Pages from: 8742  to: 8742

More Information: We would like to acknowledge the support and expertise of the staff of the Central Laser Facility. This work was partially supported by the Extreme Light Infrastructure Project, the HiPER project, the United Kingdom Engineering and Physical Sciences Research Council (grant number EP/H012605/1) and the Science and Technology Facilities Council. The work of GG has received partial funding from the European Research Council under the European Community\’s Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no. 256973.
KeyWords: Low-mass stars; Ultrashort; Fluids and Plasma physics; Electron-trasport; T-Dwarfs
DOI: 10.1038/ncomms9742

Citations: 10
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English