Massive Graviton Geons
Katsuki Aoki, Kei-ichi Maeda, Yosuke Misonoh, and Hirotada Okawa

TL;DR
This paper introduces the concept of massive graviton geons, self-gravitating bound states of massive gravitons in bigravity theory, analyzing their solutions, stability, and potential implications for dark matter and spacetime stability.
Contribution
It presents the first vacuum solutions for massive graviton geons, including non-spherical configurations, and investigates their stability and possible physical relevance.
Findings
Existence of non-spherical and spherical graviton geon solutions.
The non-spherical solution has lower energy eigenvalue, indicating it as the ground state.
The spherical solution exhibits an unstable quadrupole mode, suggesting a transition to the non-spherical state.
Abstract
We find vacuum solutions such that massive gravitons are confined in a local spacetime region by their gravitational energy in asymptotically flat spacetimes in the context of the bigravity theory. We call such self-gravitating objects massive graviton geons. The basic equations can be reduced to the Schr\"odinger-Poisson equations with the tensor "wavefunction" in the Newtonian limit. We obtain a non-spherically symmetric solution with as well as a spherically symmetric solution with in this system where is the total angular momentum quantum number and is the orbital angular momentum quantum number, respectively. The energy eigenvalue of the Schr\"odinger equation in the non-spherical solution is smaller than that in the spherical solution. We then study the perturbative stability of the spherical solution and find that there is an unstable mode in…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
