Massive Star Winds and Trajectories around Black Holes

Details Massive Star Winds and Trajectories around Black Holes Massive Star Winds and Trajectories around Black Holes

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..934..220p&link_type=abstract

FLOWS, BOUNDARIES, INTERACTIONS: Flows, Boundaries, and Interaction Workshop. AIP Conference Proceedings, Volume 934, pp. 220-2

Physics

Stellar Dynamics And Kinematics, Black Holes, Spacetime Topology, Causal Structure, Spinor Structure, Particle Emission, Solar Wind

Scientific paper

At the conference EFYRA [1] we presented the reconstructed topology of the magnetic flux lines for the solar wind and for prominences, solution of the Lorentz equations of motion for the local Minkowski spacetime of a global Dimension Embedded in Unified Symmetry (DEUS) topology of the Universe. The second solution of same equations of motion will give us the massive stars wind topology, or the followed trajectories in the proximity of a black hole distorted spacetime, differentiated after the values of the integration constants.

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