stars: neutron
Gravitational waves from accreting neutron stars and Cassiopeia A
... Chapters 5–9 are concerned with gravitational waves, and the challenge of analysing the output of kilometre-scale laser interferometric detectors in search of their signatures. In Chapter 5, we summarise results from the ...
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Prinz, Tobias (2013): Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants. Dissertation, LMU München: Fakultät für Physik
... two neutron stars or a neutron star with a black hole would yield the masses of the two gravitating bodies as well as the radius of the NS (Lattimer and Prakash, ...two neutron stars in ...
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Neutron stars velocities and magnetic fields
... We have studied a model that can explain the observations of large velocities found on neutron stars. Our model is based on the magnetic induced anisotropic emission of neutrinos as a mechanism of ...
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Evolution of Neutron Stars and Observational Constraints
... of neutron stars is discussed with a view towards constraining the prop- erties of high density matter through ...of neutron stars is illuminated through the use of several analytical ...
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The Magnetospheres of (Accreting) Neutron Stars - Observational Clues
... on neutron stars and to serve as an introduction to the more specialized contributions in these ...how neutron stars in X-ray binary systems accrete matter from their donor stars, while ...
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Dynamical Stability of Nascent Neutron Stars
... Dynamical Stability of Nascent Neutron Stars Thesis by Yuk Tung Liu In Partial Fulfillment of the Requirements for the Degree of Doct or of Philosophy California Institute of Technology P asaden a, Ca[.] ...
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From nuclear structure to neutron stars
... above, neutron star radius measurements have proven more di ffi cult, because they require both a distance measurement and some degree of modeling of the neutron star X-ray ...are neutron ...
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The Equation of State of Nuclear Matter and Neutron Stars Properties
... study neutron star observables such as the mass-radius ...studding neutron star properties: 1) It must display the correct saturation point for symmetric nuclear matter (SNM); 2) It must give a symmetry ...
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The Formation and Evolution of Neutron Stars: Astrometry, Timing, and Transients
... The discovery of ‘SGR-like’ outbursts from 1E 2259+586 was the first direct ev- idence of the connection between SGRs and AXPs (Kaspi et al. 2003). However, the nature of the relation based on indirect evidence, such as ...
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Constraining gravity with hadron physics: neutron stars, modified gravity and gravitational waves
... fective Theory is generated order by order in the chiral expansion (a low-momentum, small pion- mass expansion). It offers a measure of control over the order at which more complicated potential terms and relativistic, ...
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What can neutron stars reveal about the equation of state of dense matter?
... Abstract. Neutron stars are astrophysical objects of extremes, reaching the highest den- sities we can observe in the cosmos, and probing matter under conditions that cannot be recreated in terrestrial ...
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The Creation of Neutron Stars and Black Stars and How the Chandrasekhar Limit Prevents the Creation of Intermediate Black Stars
... Using the model created in Excel, it was found that during a supernova explo- sion, the remnant core, with a mass between 1.4 and 2 solar masses, would con- tract down to a neutron star. Stellar black stars ...
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Constructing neutron stars with a gravitational Higgs mechanism
... Before closing we would like to stress that generating a mass for the photon via spontaneous symmetry breaking within the standard model might require a more elabo- rate model than the one considered here in order to ...
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Interplay of antikaons with hyperons in nuclei and in neutron stars
... in neutron stars is investigated based on the same interaction model within the relativistic mean-field ...In neutron stars, on the other hand, kaon condensation appears in hyperon-mixed ...
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Formation and Evolution of Neutron Star Binaries: Masses of Neutron Stars
... independent of the maximum mass of NS, but the result of evolution of NS binaries. We discuss that NS-NS binaries are formed when the initial mass di ff erence of two progenitors of double neutron stars is ...
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Neutrino Processes in Neutron Stars
... of neutron stars and to show how to calculate the neutrino production rate in dense strongly interacting nuclear ...in neutron stars is subject of strong modifications due to collective effects ...
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Delta isobars in neutron stars
... hadronic stars and quark stars a very important issue must be addressed: there is no clear evidence of strangelets in cosmic ...quark stars do exist it is conceivable that quark stars mergers ...
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The diversity of neutron stars: nearby thermally emitting neutron stars and the compact central objects in supernova remnants
... radio-quiet neutron stars, and long-period radio pulsars with high inferred magnetic fields (HBPSR) are now routinely found in astronomical ...of neutron stars have primarily come from ...
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Equation of State of Dense Matter and Consequences for Neutron Stars
... In summary, taking into account the full tensor structure of the vector-meson-baryon couplings in a Hartree-Fock treatment of the QMC model gives increased pressure at high density — largely because of the ρN tensor ...
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Accreting neutron stars and black holes
... The sporadic outbursts are thought to be triggered by thermal-viscous instabilities in the accretion disc that leads to an increased mass accretion rate onto the compact accretor (see e.g. Lasota 2001). Dynamical studies ...
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