Discover
/
Article

Dark matter may slow pulsars’ spin

JUN 24, 2014
Physics Today

New Scientist : Observations have revealed that many pulsars—the superdense, rapidly rotating neutron stars left following a star as it goes nova—have slowing rotations. Chris Kouvaris of the University of Southern Denmark and Maria Ángeles Pérez-García at the University of Salamanca in Spain propose that some of the slowdown is caused by the form of dark matter known as WIMPs, weakly interacting massive particles. WIMPs have a slight electric charge, which causes them to become trapped by pulsars’ magnetic fields. Once enough charge has accumulated, it is released along the magnetic field’s poles as an electric current. The interaction between the current and the magnetic field would slow the pulsar’s spin. Kouvaris and Pérez-García say that the theory can be tested by comparing pulsars at different distances from galactic centers. The pulsars closer to larger densities of dark matter would probably have faster slowdown rates.

Related content
/
Article
The physicist-philosopher’s work on understanding climate change is also relevant for adaptation measures in health, law, and the economy.
/
Article

Get PT newsletters in your inbox

pt_newsletter_card_blue.png
PT The Week in Physics

A collection of PT's content from the previous week delivered every Monday.

pt_newsletter_card_darkblue.png
PT New Issue Alert

Be notified about the new issue with links to highlights and the full TOC.

pt_newsletter_card_pink.png
PT Webinars & White Papers

The latest webinars, white papers and other informational resources.

By signing up you agree to allow AIP to send you email newsletters. You further agree to our privacy policy and terms of service.