The Quantum and thermodynamic properties of dyonic RN-like black holes

The effect of magnetic fields on black hole superradiance is an exciting topic with possible astrophysical applications. A dyonic RN-like black hole is not asymptotically flat. It describes a black hole immersed in an asymptotically uniform magnetic field. This paper discusses the superadditive stability of binary RN black holes, asymptotically flat, band-like black holes. This article introduces the above condition into dyonic RN-like black holes if a dyonic RN-like black hole satisfies the requirement of $\mu =y\omega$, When $\sqrt{2(B^2+Q^2)}\mathrm{/}{r}_{+}^2<\omega <q{\Phi }_H$,particularly $\mu \ge \sqrt{2}(q{\Phi }_H)$,the dyonic RN-like black hole is superradiantly stable at that time.Scalars can be seen as combinations of positive/negative powers of a base, much like the decimal system. This principle is key in math and computing, from number systems to Fourier series (linked to $e^{ix}$ ). Dyonic RN-like black holes show no phase transition.