2021
DOI: 10.3390/universe7090325
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A Relativistic Entropic Hamiltonian–Lagrangian Approach to the Entropy Production of Spiral Galaxies in Hyperbolic Spacetime

Abstract: Double-spiral galaxies are common in the Universe. It is known that the logarithmic double spiral is a Maximum Entropy geometry in hyperbolic (flat) spacetime that well represents an idealised spiral galaxy, with its central supermassive black hole (SMBH) entropy accounting for key galactic structural features including the stability and the double-armed geometry. Over time the central black hole must accrete mass, with the overall galactic entropy increasing: the galaxy is not at equilibrium. From the associa… Show more

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Cited by 14 publications
(29 citation statements)
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“…( 6) & (9). Note that entropy production as such was similarly handled analytically by Parker & Jeynes [3], and an isomorphism between the Schrödinger equation and an entropic Partition Function was also specified (by Parker & Jeynes [6], their Eq.15) from the geometrical (QGT) perspective.…”
Section: Isomorphism Between Quantum Mechanics and Statistical Mechanicsmentioning
confidence: 99%
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“…( 6) & (9). Note that entropy production as such was similarly handled analytically by Parker & Jeynes [3], and an isomorphism between the Schrödinger equation and an entropic Partition Function was also specified (by Parker & Jeynes [6], their Eq.15) from the geometrical (QGT) perspective.…”
Section: Isomorphism Between Quantum Mechanics and Statistical Mechanicsmentioning
confidence: 99%
“…( 4)). But even though black holes appear to be non-conservative systems, Parker & Jeynes [3] have proved that entropy production Π is a Noether-conserved quantity. In all these cases, and in many others, the system geometry entails the conservation laws, whether or not dissipation is present.…”
Section: Irreversibility As An Intrinsic Property Of the Physical Realmmentioning
confidence: 99%
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