Metric-Independent Volume-Forms in Gravity and Cosmology
Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

TL;DR
This paper explores the use of alternative, metric-independent volume-forms in gravity and cosmology, revealing new mechanisms for cosmological constant generation, inflation, and supersymmetry breaking, with detailed Hamiltonian analysis.
Contribution
It introduces a class of gravity-matter models with two independent non-Riemannian volume-forms, demonstrating their physical implications and canonical structure.
Findings
New mechanism for dynamical cosmological constant
Emergent universe scenario before inflation
Spontaneous supersymmetry breaking in supergravity
Abstract
Employing alternative spacetime volume-forms (generally-covariant integration measure densities) independent of the pertinent Riemannian spacetime metric have profound impact in general relativity. Although formally appearing as "pure-gauge" dynamical degrees of freedom they trigger a number of remarkable physically important phenomena such as: (i) new mechanism of dynamical generation of cosmological constant; (ii) new type of "quintessential inflation" scenario in cosmology; (iii) non-singular initial "emergent universe" phase of cosmological evolution preceding the inflationary phase; (iv) new mechanism of dynamical spontaneous breakdown of supersymmetry in supergravity; (v) gravitational electrovacuum "bags". We study in some detail the properties, together with their canonical Hamiltonian formulation, of a class of generalized gravity-matter models built with two independent…
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.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
