| Literature DB >> 27231195 |
Nestor D Bareza1, Nathaniel Hermosa1.
Abstract
That the speed of light in free space c is constant has been a pillar of modern physics since the derivation of Maxwell and in Einstein's postulate in special relativity. This has been a basic assumption in light's various applications. However, a physical beam of light has a finite extent such that even in free space it is by nature dispersive. The field confinement changes its wavevector, hence, altering the light's group velocity vg. Here, we report the subluminal vg and consequently the dispersion in free space of Laguerre-Gauss (LG) beam, a beam known to carry orbital angular momentum. The vg of LG beam, calculated in the paraxial regime, is observed to be inversely proportional to the beam's divergence θ0, the orbital order ℓ and the radial order p. LG beams of higher orders travel relatively slower than that of lower orders. As a consequence, LG beams of different orders separate in the temporal domain along propagation. This is an added effect to the dispersion due to field confinement. Our results are useful for treating information embedded in LG beams from astronomical sources and/or data transmission in free space.Entities:
Year: 2016 PMID: 27231195 PMCID: PMC4882591 DOI: 10.1038/srep26842
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1(a) LG beam spreading through propagation and (b) LG wavefront for and p = 0.
Figure 2Colormap of v/c values as function of and p with central wavelength λ0 = 632.8 nm and minimum beam waist w0 = 2.0 μm.
Each pixel of a specific color corresponds to v/c value (colored scale bar). Warm colored pixels have relatively higher v/c values compared to cool colored pixels.
Figure 3Plots of (a) v/c versus for different p values and (b) v/c versus p for different values.
Some combinations of mode indices yielding degenerate v values of LG beam in order.
| Order | Degeneracy counts | Mode indices |
|---|---|---|
| 1 | 2 | (1, 0), (−1, 0) |
| 2 | 3 | (2, 0), (−2, 0), (0, 1) |
| 3 | 4 | (3, 0), (−3, 0), (−1, 1), (1, 1) |
| 4 | 5 | (4, 0), (−4, 0), (2, 1), (−2, 1), (0, 2) |