A new two-faced scalar solution and cosmological SUSY breaking
Marina Shmakova, Valentin Burov

TL;DR
This paper introduces a novel scalar field solution in an expanding universe that potentially explains the coexistence of supersymmetry breaking and a small cosmological constant by linking scalar mass scales to the Hubble parameter.
Contribution
It presents a new non-perturbative scalar field solution with dual-frequency behavior, connecting cosmological expansion to supersymmetry breaking and vacuum energy.
Findings
Scalar field solution exhibits dual-frequency behavior.
Mass scales are related to Hubble parameter as H^(1/4) and H^(1/2).
Proposes a mechanism for small cosmological constant and heavy scalar partners.
Abstract
We propose a possible new way to resolve the long standing problem of strong supersymmetry breaking coexisting with a small cosmological constant. We consider a scalar component of a minimally coupled N=1 supermultiplet in a general Friedmann-Robertson-Walker (FRW) expanding universe. We argue that a tiny term, proportional to H^2 ~ 10^(-122) in Plank's units, appearing in the field equations due to this expansion will provide both, the small vacuum energy and the heavy mass of the scalar supersymmetric partner. We present a non-perturbative solution for the scalar field with an unusual dual-frequency behavior. This solution has two characteristic mass scales related to the Hubble parameter as H^(1/4) and H^(1/2) measured in Plank's units.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena
