On the possibility of detecting phase transitions in the cores of accreting x-ray neutron stars<footnote id="*" pos="affil">Based on a collaboration with F Weber [1].</footnote>On the possibility of detecting phase transitions in the cores of accreting x-r

Details On the possibility of detecting phase transitions in the cores of accreting x-ray neutron stars<footnote id="*" pos="affil">Based on a collaboration with F Weber [1].</footnote>On the possibility of detecting phase transitions in the cores of accreting x-r On the possibility of detecting phase transitions in the cores of accreting x-ray neutron stars<footnote id="*" pos="affil">Based on a collaboration with F Weber [1].</footnote>On the possibility of detecting phase transitions in the cores of accreting x-r

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jphg...28.2023g&link_type=abstract

Journal of Physics G: Nuclear and Particle Physics, Volume 28, Issue 7, pp. 2023-2027 (2002).

Physics

3

Scientific paper

Phase transitions can be triggered by a change of density profile in neutron stars as a result of spin-up caused by mass accretion from a companion star. Such a spin evolution is the pathway from old canonical pulsars to millisecond pulsars. A number of x-ray neutron stars have been recently observed by the Rossi x-ray timing explorer (RXTE). Most of their frequencies are clustered in a narrow band with a few at higher frequency. This is the expected signature of a phase transition in the stellar core.

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