Yayınlanmış 1 Ocak 2012 | Sürüm v1
Dergi makalesi Açık

Spin down of rotating compact magnetized strange stars in general relativity

Açıklama

We find that in general relativity slow down of the pulsar rotation due to the magnetodipolar radiation is more faster for the strange star with comparison to that for the ordinary neutron star of the same mass. Comparison with astrophysical observations on pulsars spindown data may provide an evidence for the strange star existence and, thus, serve as a test for distinguishing it from the neutron star.

Dosyalar

bib-1a62e6a4-f18b-4c04-b238-797585a7860e.txt

Dosyalar (178 Bytes)

Ad Boyut Hepisini indir
md5:7208b120f9a32dad07867cde66da2e3f
178 Bytes Ön İzleme İndir