- Conference date: 22–27 April 2012
- Location: Bento Gonçalves, Rio Grande do Sul, Brazil
Recently, a new view of SGRs/AXPs expressed in terms of massive highly magnetized rotating white dwarfs (WDs) in total analogy with the case of pulsars originating their energy from the rotational energy of the neutron stars has been presented. Furthermore, we present the recent discoveries of two SGRs with low magnetic field sharing some properties with the recent detected fast WD pulsar AE Aquarii, to support the description of SGRs/AXPs as white dwarf pulsar. In order to test this new view, we present several properties of these SGRs/AXPs as WD pulsar, in particular the X-ray luminosity and surface dipole magnetic field.
- White dwarfs
- Magnetic fields
- Stellar magnetic fields
- Magnetic field sensors
Daniel Baumann, Mark G. Jackson, Peter Adshead, Alexandre Amblard, Amjad Ashoorioon, Nicola Bartolo, Rachel Bean, Maria Beltrán, Francesco de Bernardis, Simeon Bird, Xingang Chen, Daniel J. H. Chung, Loris Colombo, Asantha Cooray, Paolo Creminelli, Scott Dodelson, Joanna Dunkley, Cora Dvorkin, Richard Easther, Fabio Finelli, Raphael Flauger, Mark P. Hertzberg, Katherine Jones‐Smith, Shamit Kachru, Kenji Kadota, Justin Khoury, William H. Kinney, Eiichiro Komatsu, Lawrence M. Krauss, Julien Lesgourgues, Andrew Liddle, Michele Liguori, Eugene Lim, Andrei Linde, Sabino Matarrese, Harsh Mathur, Liam McAllister, Alessandro Melchiorri, Alberto Nicolis, Luca Pagano, Hiranya V. Peiris, Marco Peloso, Levon Pogosian, Elena Pierpaoli, Antonio Riotto, Uroš Seljak, Leonardo Senatore, Sarah Shandera, Eva Silverstein, Tristan Smith, Pascal Vaudrevange, Licia Verde, Ben Wandelt, David Wands, Scott Watson, Mark Wyman, Amit Yadav, Wessel Valkenburg and Matias Zaldarriaga
Data & Media loading...
Article metrics loading...