Dvali theorized that the leakage of these particles between branes is the source of dark energy, and this particle's supersymmetric partner obeys the Rarita-Schwinger equation, and, if it's the lightest supersymmetric partner and R-parity is conserved, said partner is stable. Penrose derived the existence of nonlinear ones of these from general curved twistor spaces in one seminal paper. In string theory, Schwarz and Scherk noted that this particle corresponds to a vibra
Dvali theorized that the leakage of these particles between branes is the source of dark energy, and this particle's supersymmetric partner obeys the Rarita-Schwinger equation, and, if it's the lightest supersymmetric partner and R-parity is conserved, said partner is stable. Penrose derived the existence of nonlinear ones of these from general curved twistor spaces in one seminal paper. In string theory, Schwarz and Scherk noted that this particle corresponds to a vibrating closed string at Planck tension. It is a massless spin-2 boson, and a planet-sized detector next to a neutron star would take 10 years to detect even one of these particles, which are responsible for curving spacetime according to general relativity. For 10 points, name this hypothetical particle, the carrier of the gravitational force.
Dvali theorized that the leakage of these particles between branes is the source of dark energy, and this particle's supersymmetric partner obeys the Rarita-Schwinger equation, and, if it's the lightest supersymmetric partner and R-parity is conserved, said partner is stable.
{Graviton}