TY - JOUR
T1 - Towards the Ronchi test for gravitational lenses
T2 - The gravitoronchigram
AU - Bretón, Nora
AU - Cabrera-Rosas, Omar De Jesús
AU - Espíndola-Ramos, Ernesto
AU - Juárez-Reyes, Salvador Alejandro
AU - Julián-Macías, Israel
AU - Montiel, Ariadna
AU - Ortega-Vidals, Paula
AU - Román-Hernández, Edwin
AU - Silva-Ortigoza, Gilberto
AU - Silva-Ortigoza, Ramón
AU - Sosa-Sánchez, Citlalli Teresa
AU - Suárez-Xique, Román
N1 - Publisher Copyright:
© 2017 IOP Publishing Ltd.
PY - 2017/6
Y1 - 2017/6
N2 - The aim of this work is to present a Ronchi test for a gravitational lens. To this end, we use the geometrical optics point of view of the Ronchi test and the definition of the exact lens equation without reference to a background space-time to introduce the analog of the ideal ronchigram, which we named the gravitoronchigram. We first present the ideal ronchigram for an axicon lens and then using the space-time perspective of the lensing phenomenon we obtain analytical equations of the ideal gravitoronchigram for the Schwarzschild lens in the thin lens approximation and in an exact way. Finally, because the caustic associated with the deflected light by the axicon and the Schwarzschild lenses is a line along the optical axis we conjecture the generation of a gravitoBessel beam by illuminating the Schwarzschild lens with a point light source analogous to that generated by an axicon lens. That is, a particular example of the so-called non-diffracting light fields.
AB - The aim of this work is to present a Ronchi test for a gravitational lens. To this end, we use the geometrical optics point of view of the Ronchi test and the definition of the exact lens equation without reference to a background space-time to introduce the analog of the ideal ronchigram, which we named the gravitoronchigram. We first present the ideal ronchigram for an axicon lens and then using the space-time perspective of the lensing phenomenon we obtain analytical equations of the ideal gravitoronchigram for the Schwarzschild lens in the thin lens approximation and in an exact way. Finally, because the caustic associated with the deflected light by the axicon and the Schwarzschild lenses is a line along the optical axis we conjecture the generation of a gravitoBessel beam by illuminating the Schwarzschild lens with a point light source analogous to that generated by an axicon lens. That is, a particular example of the so-called non-diffracting light fields.
KW - classical black holes
KW - geometrical optics
KW - gravitational lenses
KW - lenses
KW - prisms and mirrors
KW - relativity and gravitation
UR - http://www.scopus.com/inward/record.url?scp=85020287406&partnerID=8YFLogxK
U2 - 10.1088/2040-8986/aa6cc7
DO - 10.1088/2040-8986/aa6cc7
M3 - Artículo
SN - 2040-8978
VL - 19
JO - Journal of Optics (United Kingdom)
JF - Journal of Optics (United Kingdom)
IS - 6
M1 - 065602
ER -