Si:P as a laboratory analogue for hydrogen on high magnetic field white dwarf stars

56Citations
Citations of this article
77Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Laboratory spectroscopy of atomic hydrogen in a magnetic flux density of 10 5 T (1 gigagauss), the maximum observed on high-field magnetic white dwarfs, is impossible because practically available fields are about a thousand times less. In this regime, the cyclotron and binding energies become equal. Here we demonstrate Lyman series spectra for phosphorus impurities in silicon up to the equivalent field, which is scaled to 32.8 T by the effective mass and dielectric constant. The spectra reproduce the high-field theory for free hydrogen, with quadratic Zeeman splitting and strong mixing of spherical harmonics. They show the way for experiments on He and H 2 analogues, and for investigation of He 2, a bound molecule predicted under extreme field conditions. © 2013 Macmillan Publishers Limited.

Cite

CITATION STYLE

APA

Murdin, B. N., Li, J., Pang, M. L. Y., Bowyer, E. T., Litvinenko, K. L., Clowes, S. K., … Murdin, P. G. (2013). Si:P as a laboratory analogue for hydrogen on high magnetic field white dwarf stars. Nature Communications, 4. https://doi.org/10.1038/ncomms2466

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free