We demonstrate high-speed silicon modulators optimized for operating at the wavelength of 2 μm. The Mach-Zehnder interferometer (MZI) carrier-depletion modulator with 2 mm phase shifter has a single-arm modulation efficiency (V ·L) of 2.89 V·cm at 4 V reverse bias. Using a push-pull configuration it operates at a data rate of 25 Gbit/s OOK with an extinction ratio of 6.25 dB. We also proposed a mathematically-analysed streamlined IMDD PAM-4 scheme and successfully demonstrated a 25 Gbit/s datarate PAM-4 with the same 2 mm modulator. A Michelson interferometer carrier-depletion modulator with 0.5 mm phase shift length has also been shown with modulation efficiency (V ·L) of 1.36 V·cm at 4 V reverse bias and data rate of 20 Gbit/s OOK. The Michelson interferometer modulator performs similarly to a Mach-Zehnder modulator with twice the phase shifter length.

Download full-text PDF

Source
http://dx.doi.org/10.1364/OE.418285DOI Listing

Publication Analysis

Top Keywords

michelson interferometer
12
modulator phase
12
high-speed silicon
8
interferometer modulator
8
streamlined imdd
8
imdd pam-4
8
carrier-depletion modulator
8
phase shifter
8
modulation efficiency
8
efficiency v ·l
8

Similar Publications

In this Letter, we present a fiber-optic radio frequency (RF) transmission scheme based on phase modulation with an interferometric detection structure. A self-developed Michelson interferometer (MI) is used to demodulate the frequency signal via an electrically controlled optical shifter. The two complementary outputs from the interferometer are detected using a balanced detector, which suppresses the common-mode noise of the fiber link.

View Article and Find Full Text PDF

High-Performance Telescope System Design for Space-Based Gravitational Waves Detection.

Sensors (Basel)

November 2024

MOE Key Laboratory of Fundamental Physical Quantities Measurement and Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, China.

Article Synopsis
  • Space-based gravitational wave (GW) detection utilizes the Michelson interferometry principle to create long baseline laser interferometers capable of sensing signals within a frequency range of 10-1 Hz.
  • The paper introduces an advanced design using an off-axis four-mirror configuration that minimizes wavefront aberration and enhances stray light suppression, addressing background noise issues.
  • This improved design achieves a wavefront error of less than λ/500 in the main field of view and can reach an error of less than λ/30 with a 92% probability, making it a strong candidate for future GW detection projects.
View Article and Find Full Text PDF

Atmospheric temperature information in the near space is of great academic significance and engineering value to support the development and utilization of the near space. Based on the theory of O molecular dayglow spectroscopy and the mechanism of atmospheric radiative transfer, a method is proposed for the joint retrieval of temperature profiles in the near space using O(aΔ) and O(b∑ ) bands dayglow spectroscopy signal with the self-absorption effect. First, the temperature dependence of O(aΔ) and O(b∑ ) bands dayglow is investigated, and the influence of the self-absorption effect on the radiative transfer characteristics is analyzed in the limb-view mode.

View Article and Find Full Text PDF

We present a low-resource and robust optical implementation of the four-dimensional Grover coin, a four-port linear-optical scatterer that augments the low dimensionality of a regular beam-splitter. While prior realizations of the Grover coin required a potentially unstable ring cavity to be formed, this version of the scatterer does not exhibit any internal interference. When this Grover coin is placed in another system, it can be used for interferometry with a higher-dimensional set of optical field modes.

View Article and Find Full Text PDF

Significance: Optical coherence tomography (OCT) images are prone to image artifacts due to the birefringence of the sample or the optical system when a polarized light source is used for imaging. These artifacts can lead to degraded image quality and diagnostic information.

Aim: We aim to mitigate these birefringence-related artifacts in OCT images by adding a depolarizer module in the reference arm of the interferometer.

View Article and Find Full Text PDF

Want AI Summaries of new PubMed Abstracts delivered to your In-box?

Enter search terms and have AI summaries delivered each week - change queries or unsubscribe any time!