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M. L. Deglmann

Publications and source records attributed to M. L. Deglmann.

3 recordsLinked to original sources

Extended Scalar Particle Solutions in Black String Spacetimes with Anisotropic Quintessence

We present novel solutions to the Klein-Gordon equation in a black string spacetime immersed in an anisotropic quintessence fluid and surrounded by a cloud of strings (BCK spacetime). The solutions are shown to depend on the quintessence state parameter $α_{Q}$ and extend to a broader radial domain than previously reported. Explicit analytical results are provided for $α_{Q} = 0, 1/2, 1$, thereby encompassing all relevant physical scenarios. These analytical radial solutions are derived using the confluent and biconfluent Heun equations, as well as Bessel equations in specific cases. Constraints on the Heun parameters that produce spectral restrictions are examined, resulting in the $δ_{N}-$subclass of solutions, which includes the polynomial cases. Quintessence-induced \enquote{dark phases} are identified for several scenarios; in particular, the regime of $α_{Q} = 1$ is emphasized for future comparison with alternative spacetime geometries. These findings contribute to the understanding of scalar particle dynamics and the influence of dark energy on quantum systems in curved spacetime backgrounds.

gr-qc

Emergence of Dark Phases in Scalar Particles within the Schwarzschild-Kiselev-Letelier Spacetime

This work focuses on the emergence of dark phases (dark energy-induced phases) in the radial wave function of scalar particles. We achieve this by presenting novel solutions to the Klein-Gordon equation in a spherically symmetric spacetime, which encompasses a black hole, a quintessential fluid, and a cloud of strings. We determine the exact solution for the spacetime metric, analyze the admissible ranges for its physical parameters, and discuss the formation of the event horizon. Subsequently, we detail the solution of the Klein-Gordon equation and explore three distinct cases of dark phases, corresponding to the quintessence state parameter $α_{Q}$ taking the values $0$, $1/2$, and $1$. Notably, the case where $α_{Q} = 1$ holds particular significance due to current observational constraints on dark energy.

gr-qc

Asymptotic Stability Analysis for $SU(n)$ Dark Monopoles

We analyze the asymptotic stability of the $SU(n)$ Dark Monopole solutions and we show that there are unstable modes associated with them. We obtain the explicit form of the unstable perturbations and the associated negative-squared eigenfrequencies.

hep-th