Self-aligned non-dispersive external cavity
tunable laser
Christoph e Mose r,
1,*
Lawrence Ho,
2
and Frank Havermeyer
3
1,2,3
Ondax, Inc., 850 E. Duarte Road, Monrovia, CA, 91016, USA
*
Corresponding author: moser@ondax.com
Abstract: We are reporting on a novel self-aligned non-dispersive external
cavit y laser (ECL) based on thic k volume hologra phic grat ings (VHG) . The
ECL is tunable and operates with single mode and broad area multimode
laser diodes. We experimentally demonstrate tunable single frequency
operation at 405 nm and 785 nm. The tunable ECL concept is also
experimentally tested with high power broad area laser diodes near 780 nm.
The passive alignment feature of the cavity is expected to reduce the
assembly cost of tunable ECLs.
©2008 Optical Societ y of America
OCIS codes: (140;2020) Diode lasers; (090.4220) Multiplex holography
References and links
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expanders,” J. Light wave Technol. 10, 3, pp. 330-335. (1992).
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1. Introduction
State-of-the-art Littrow and Littman external cavity lasers (ECL) use an angularly dispersive
surface diffraction grating as the frequency selective element and a rotation scheme to provide
wavelength tuning [1,2,3]. Although miniaturization of ECLs have been attempted
commercially at the 1.5 μm telecommunication wavelength using MEMs to rotate the
components [4], footprint reduction has been difficult to realize at shorter wavelength. The
#101190 - $15.00 USD Received 5 Sep 2008; revised 1 Oct 2008; accepted 2 Oct 2008; published 3 Oct 2008
(C) 2008 OSA 13 October 2008 / Vol. 16, No. 21 / OPTICS EXPRESS 16691
main reason is that shorter wavelength requires higher spectral resolution and this tends to
increa se the size o f the optic s.
In contrast to the Littman and Littrow cavities, fixed wavelength ECLs using non-
disp e rsive re f le ctio n volume ho lo gra ph ic gr a tings ( VHG) h a ve be e n re por te d f or t he f irst time
to the authors’ knowledge in 1985 [5]. Since then, others have made fixed wavelength ECLs
using VHGs for single mode and multimode high power lasers [6-9]. Although passive
alignment of an ECL with VHGs has been demonstr ated [8], such an ECL is tu nable only by
controlling the temperature of the VHG, which limits the tuning range to a few tenths of a
nanometer. The current study demonstrates both passive alignment and large tuning range
using VHGs.
2. Comparison of the spectral resolution of ECL with dispersive and non-dispersive
gratings.
In the Littrow cavity (Fig.1(a))the diffraction grating, typically blazed, retro-reflects the
diffraction order back in the direction approximately opposite to the incoming collimated
beam. The zero order of the diffraction is the output of the cavity. Schemes to stabilize the
alignment sensitivity have been devised by introducing optical elements such as cylindrical
lenses between the collimated lens and the diffraction grating [2]. A disadvantage of the
Littrow cavity is that angular tuning of the diffraction grating also changes the direction of the
output beam. The spectral resolution of the Littrow laser cavity is given by [10].
βπ
λ
λ
tan
2
o
Littrow
D
=Δ
, (1)
where
λ
is the wavelength of the laser,
o
D is the diameter of the collimated beam at the
waist and
β
is the angle formed by the normal of the dispersive grating and the direction of
the co llimated beam. As can be noted fro m equatio n 1, for ma ximum spe ctral re solution, the
diameter of the beam should be as large as possible and at a grazing angle on the dispersive
grating. A larger beam diameter increases the cavity length since either a longer focal length
or intracavity prism expanders [3] are required.
VHG
L
Laser Diode
D ispersive grating
Laser Diode
D
o
β
λ
1
λ
2
(a)
(b)
VHG
L
Laser Diode
VHG
L
Laser Diode
D ispersive grating
Laser Diode
D
o
β
λ
1
λ
2
(a)
(b)
Fig. 1. (a) Littrow ECL with dispersive grati ng (b) EC L based on non- dispers i ve VHGs.
Figure 1(b) shows an ECL based on a non-dispersive VHG for the spectrally
selective component in the cavity [5]. The VHG acts as a narrowband reflective output
#101190 - $15.00 USD Received 5 Sep 2008; revised 1 Oct 2008; accepted 2 Oct 2008; published 3 Oct 2008
(C) 2008 OSA 13 October 2008 / Vol. 16, No. 21 / OPTICS EXPRESS 16692