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Polarized x-rays from a magnetar

Authors :
Taverna, Roberto
Turolla, Roberto
Muleri, Fabio
Heyl, Jeremy
Zane, Silvia
Baldini, Luca
Caniulef, Denis González
Bachetti, Matteo
Rankin, John
Caiazzo, Ilaria
Di Lalla, Niccolò
Doroshenko, Victor
Errando, Manel
Gau, Ephraim
Kırmızıbayrak, Demet
Krawczynski, Henric
Negro, Michela
Ng, Mason
Omodei, Nicola
Tamagawa, Toru
Uchiyama, Keisuke
Weisskopf, Martin C.
Agudo, Ivan
Antonelli, Lucio A.
Baumgartner, Wayne H.
Bellazzini, Ronaldo
Bianchi, Stefano
Bongiorno, Stephen D.
Bonino, Raffaella
Brez, Alessandro
Bucciantini, Niccolò
Capitanio, Fiamma
Castellano, Simone
Cavazzuti, Elisabetta
Ciprini, Stefano
Costa, Enrico
De Rosa, Alessandra
Del Monte, Ettore
Di Gesu, Laura
Di Marco, Alessandro
Donnarumma, Immacolata
Dovčiak, Michal
Ehlert, Steven R.
Enoto, Teruaki
Evangelista, Yuri
Fabiani, Sergio
Ferrazzoli, Riccardo
Garcia, Javier A.
Gunji, Shuichi
Hayashida, Kiyoshi
Iwakiri, Wataru
Jorstad, Svetlana G.
Karas, Vladimir
Kitaguchi, Takao
Kolodziejczak, Jeffery J.
La Monaca, Fabio
Latronico, Luca
Liodakis, Ioannis
Maldera, Simone
Manfreda, Alberto
Marin, Frédéric
Marinucci, Andrea
Marscher, Alan P.
Marshall, Herman L.
Matt, Giorgio
Mitsuishi, Ikuyuki
Mizuno, Tsunefumi
Ng, Stephen C. -Y.
O'Dell, Stephen L.
Oppedisano, Chiara
Papitto, Alessandro
Pavlov, George G.
Peirson, Abel L.
Perri, Matteo
Pesce-Rollins, Melissa
Pilia, Maura
Possenti, Andrea
Poutanen, Juri
Puccetti, Simonetta
Ramsey, Brian D.
Ratheesh, Ajay
Romani, Roger W.
Sgrò, Carmelo
Slane, Patrick
Soffitta, Paolo
Spandre, Gloria
Tavecchio, Fabrizio
Tawara, Yuzuru
Tennant, Allyn F.
Thomas, Nicolas E.
Tombesi, Francesco
Trois, Alessio
Tsygankov, Sergey
Vink, Jacco
Wu, Kinwah
Xie, Fei
Publication Year :
2022

Abstract

We report on the first detection of linearly polarized x-ray emission from an ultra-magnetized neutron star with the Imaging X-ray Polarimetry Explorer (IXPE). The IXPE 35 observations of the anomalous x-ray pulsar 4U 0142+61 reveal a linear polarization degree of $(12\pm 1)\%$ throughout the IXPE 2--8 keV band. We detect a substantial variation of the polarization with energy: the degree is $(14\pm 1)\%$ at 2--4 keV and $(41\pm 7)\%$ at 5.5--8 keV, while it drops below the instrumental sensitivity around 4--5 keV, where the polarization angle swings by $\sim 90^\circ$. The IXPE observations give us completely new information about the properties of the neutron star surface and magnetosphere and lend further support to the presence of the quantum mechanical effect of vacuum birefringence.<br />Comment: 32 pages, 9 figures, 3 tables

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2205.08898
Document Type :
Working Paper
Full Text :
https://doi.org/10.1126/science.add0080