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Ian Jones
(University of Southampton)
25/04/2016, 09:10
Isolated neutron stars can emit gravitational waves via a variety of mechanisms. These emission channels are highly sensitive to the nature of matter in the star, and can potentially reveal information on the high density equation of state not accessible via other means. In this talk I will review these mechanisms, and discuss how they relate to the microphysics of the stellar matter. I will...
Kostas Glampedakis
25/04/2016, 10:00
This talk will provide an update on gravitational wave emission from isolated neutron stars and on the dynamics of the associated unstable oscillation modes.
Friedrich Thielemann, Andreas Lohs
(University of Basel)
26/04/2016, 09:10
Luciano Rezzolla
(Institute for Theoretical Physics, Frankfurt, Germany)
27/04/2016, 09:10
Prof.
Chris Pethick
(University of Illinois at Urbana-Champaign)
27/04/2016, 10:00
I shall discuss a number of subjects including the equation of state of uniform nucleonic matter, collective oscillations in the inner crust of neutron stars, the neutron superfluid density in the inner crust, elastic properties of the crust, induced interactions between nucleons and the transition to quark matter.
Gergely Gabor Barnaföldi- Szilvia Karsai-Peter Posfay
(Wigner RCP Hungarian Academy of Sciences (HU))
28/04/2016, 12:10
Recently we have explored the properties of an interacting fermionic compact star in a 1+4 dimensional Kaluza--Klein-like spacetime, where an extra microscopical spacelike dimension was introduced (See Sz. Karsai's talk). Here, we present wether we would able to measure the effect of these extra dimensions by gravitational wave detectors.
Dr
Bettina Posselt
29/04/2016, 09:10
Silvia Zane
(university college London)
29/04/2016, 10:00
Multi-wavelength observations over the last decades proved the existence of observationally very diverse manifestations of isolated NSs (INSs) and led to the separation of INSs into distinct classes. Most of the ~2,300 known INSs are radio pulsars with periods P < 8 s and magnetic field B ~ 10 12 G, but there are objects with much greater potential for understanding the INSs diversity. This...
Prof.
M. Ali Alpar
(Istanbul University)
29/04/2016, 11:30
Plenary talk
Theoretical basis and observational evidence for nonlinear dynamics will be discussed.
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