Future CMOS technology is clearly moving towards digital voltage levels of 1 V. The
ITRS Roadmap indicates an expected off-chip speed of 9.5 GHz
and a voltage of
1.0 V in 2010 [1]. By 2016, the ITRS predicts
the voltage will only have dropped
to
0.8 V while
the off-chip speed
will have increased to around 36 GHz
[1]. In addition,
current long-haul and medium-haul
optical networks utilize WDM fiber-based systems
operating at a wavelength around
1550 nm and at bit rates of 10 Gbps. If the future
of both personal computing and telecommunications involves optical
networks, it seems natural to expect these two types of networks to seamlessly integrate.
In order to design a surface-normal
modulator for optical interconnects,
several factors must be taken into consideration, as
described in Chapter 3. The AlGaAs modulator from Chapter
4
achieved
a
good
contrast
ratio
of
~
6
dB for
a
5-nm- wavelength range around 850 nm, but required 2.5 V of voltage
drive. Lowering the voltage drive to 1 V reduced the contrast ratio to ~3 dB for 5 nm.
This standard
surface- normal design is subject to a
tradeoff between contrast ratio, wavelength range, and low voltage operation, discussed below.
In order
to achieve a contrast ratio
of 3 dB over a
wider wavelength range without dramatically
increasing the voltage drive, some new strategy must be employed.
These considerations, very low voltage
drive and compatibility with larger C- band WDM optical
networks, led us to design a high-speed, low-voltage modulator operating at 1550 nm. This novel modulator
architecture,
called
a quasi-waveguide angled-facet electroabsorption modulator (QWAFEM),
and its advantages will be
presented in this chapter, followed
by a description of the methods of its design, fabrication, and testing.
LOW VOLTAGE OPERATION
A surface-normal modulator that operates
on only 1 V of digital
voltage swing must be extremely thin in order to achieve a high electric field change across the MQW
region. However,
a thin MQW region results in a low contrast ratio, unless an optical resonator is implemented surrounding it, as in the AFPM discussed
in Chapter 4. As the
quality factor of the AFPM resonator is increased, the contrast ratio improves,
but the wavelength range is limited. A high contrast ratio for a low voltage swing is possible
at the expense of the wavelength range, as in [2] where a contrast
ratio of 10 dB for 1 V was
achieved across less than 1 nm of wavelength range. Note that, for a given quality factor, the wavelength range increases for
shorter cavities
It seems the ideal modulator
would have a thin MQW region
(in order to allow a large change in the electric
field for a small voltage swing) and a short Fabry-Perot
optical cavity with highly reflective mirrors (in order to achieve
a high contrast ratio
while maintaining
the maximum
possible wavelength range). Unfortunately, in a surface-normal geometry (i.e. the light propagation axis
perpendicular to the epitaxial layers), the penetration depth of dielectric mirrors can be many wavelengths on each side, making a very short optical cavity
impossible. Metallic mirrors can be utilized
instead, but they suffer from absorption.
This dilemma, the tradeoff between contrast ratio, low voltage,
and wavelength range, seems
inherent to surface-normal modulators, but it is avoided in waveguide
modulators.
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