Figure 5 | Scientific Reports

Figure 5

From: Modelling quantum aspects of disruption of a white dwarf star by a black hole

Figure 5

Density with streamlines (left frames) and the phase (right frames) of the bosonic accretion disk at different times, increasing from top to bottom. The unit of time is \((m_B a_B^2)/\hbar \). The black hole is in the (0,0) position. The quantized vortices are visible as plus and minus signs present within the matter spiraling around the black hole, at the inner and outer edges of the matter spout, as well as in the region of low density.

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