The double pulsar J0737-3039: testing the neutron star equation of state
The double pulsar J0737--3039 has become an important astrophysical laboratory for testing fundamental physics. Here we demonstrate that the low measured mass of Pulsar B can be used to constrain the equation of state of neutron star matter {\em under the assumption} that it formed in an electron-ca...
主要な著者: | Podsiadlowski, P, Dewi, J, Lesaffre, P, Miller, J, Newton, W, Stone, JR |
---|---|
フォーマット: | Journal article |
言語: | English |
出版事項: |
Oxford University Press
2005
|
類似資料
-
On the 2PN Periastron Precession of the Double Pulsar PSR J0737–3039A/B
著者:: Lorenzo Iorio
出版事項: (2021-11-01) -
Prospects of Constraining the Dense Matter Equation of State from Timing Analysis of Pulsars in Double Neutron Star Binaries: The Cases of PSR J0737 ‒ 3039A and PSR J1757 ‒ 1854
著者:: Manjari Bagchi
出版事項: (2018-02-01) -
Double-core evolution and the formation of neutron-star binaries with
compact companions
著者:: Dewi, J, 等
出版事項: (2006) -
The spin period - eccentricity relation of double neutron stars:
evidence for weak supernova kicks?
著者:: Dewi, J, 等
出版事項: (2005) -
Superresolving Distant Galaxies with Gravitational Telescopes: Keck Laser Guide Star Adaptive Optics and
Imaging of the Lens System SDSS J0737+3216
著者:: Marshall, P, 等
出版事項: (2007)