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Evidence of vacuum birefringence from the polarisation of the optical emission from an Isolated Neutron Star

Mignani, R; Testa, V; Gonzalez, D; Taverna, R; Zane, S; Wu, K; Lo Curto, D; (2017) Evidence of vacuum birefringence from the polarisation of the optical emission from an Isolated Neutron Star. In: Zioutas, K and Anastassopoulos, V, (eds.) 13th Patras Workshop on Axions, WIMPs and WISPs. (pp. pp. 163-167). Green open access

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Abstract

Isolated Neutron Stars are some of the most exciting stellar objects known to astronomers: they have the most extreme magnetic fields, with values up to 1015 G, and, with the exception of stellar-mass black holes, they are the most dense stars, with densities of ≈ 1014 g cm−3 . As such, they are perfect laboratories to test theories of electromagnetism and nuclear physics under conditions of magnetic field and density unattainable on Earth. In particular, the interaction of radiation with strong magnetic fields is the cause of the vacuum birefringence, an effect predicted by quantum electrodynamics in 1936 but that lacked an observational evidence until now. Here, we show how the study of the polarisation of the optical radiation from the surface of an isolated neutron star yielded such an observational evidence, opening exciting perspectives for similar studies at other wavelengths.

Type: Proceedings paper
Title: Evidence of vacuum birefringence from the polarisation of the optical emission from an Isolated Neutron Star
Event: 13th Patras Workshop on Axions, WIMPs and WISPs, 15 - 19 May 2017, Thessaloniki, Greece
Location: Thessaloniky Greece
Dates: 15 May 2017 - 19 May 2017
ISBN-13: 9783945931172
Open access status: An open access version is available from UCL Discovery
DOI: 10.3204/DESY-PROC-2017-02
Publisher version: https://doi.org/10.3204/DESY-PROC-2017-02
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10039120
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