In physically motivated models of quantum spacetime, a U(1) gauge theory turns into a U(infinity) gauge theory; hence, free classical electrodynamics is no longer free and neutral fields may have electromagnetic interactions. We discuss the last point for scalar fields, as a way to possibly describe dark matter; we have in mind the gravitational collapse of binary systems or future applications to self-gravitating Bose-Einstein condensates as possible sources of evidence of quantum gravitational phenomena. The effects considered so far, however, seem too faint to be detectable at present.
Doplicher, S., Fredenhagen, K., Morsella, G., Pinamonti, N. (2017). Dark matter and weak signals of quantum spacetime. PHYSICAL REVIEW D, 95(6) [10.1103/PhysRevD.95.065009].
Dark matter and weak signals of quantum spacetime
Morsella G.;
2017-01-01
Abstract
In physically motivated models of quantum spacetime, a U(1) gauge theory turns into a U(infinity) gauge theory; hence, free classical electrodynamics is no longer free and neutral fields may have electromagnetic interactions. We discuss the last point for scalar fields, as a way to possibly describe dark matter; we have in mind the gravitational collapse of binary systems or future applications to self-gravitating Bose-Einstein condensates as possible sources of evidence of quantum gravitational phenomena. The effects considered so far, however, seem too faint to be detectable at present.File | Dimensione | Formato | |
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