Archivio Istituzionale della RicercaIn this talk the different possibilities offered by light (geometric effects, polarization ef- fects, propagation delays and phase changes) for determining the local structure of space time, i.e., the gravitational field, in terms of the Riemann tensor, are discussed. Special attention is devoted to axially symmetric stationary gravitational fields. A description of the potentialities of ring lasers is presented, having direct reference to the GINGER project.
Light: a perfect probe for gravity / Tartaglia, Angelo. - STAMPA. - (2016), pp. 1-6. (Intervento presentato al convegno Fourteenth Marcel Grossmann Meeting - MG14 tenutosi a Roma nel July 12-18, 2015).
Light: a perfect probe for gravity
TARTAGLIA, Angelo
2016
Abstract
In this talk the different possibilities offered by light (geometric effects, polarization ef- fects, propagation delays and phase changes) for determining the local structure of space time, i.e., the gravitational field, in terms of the Riemann tensor, are discussed. Special attention is devoted to axially symmetric stationary gravitational fields. A description of the potentialities of ring lasers is presented, having direct reference to the GINGER project.
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https://hdl.handle.net/11583/2664173
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