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Sensing and Signal Analysis

Code: FIS4051     Acronym: FIS4051     Level: 400

Keywords
Classification Keyword
OFICIAL Physics

Instance: 2024/2025 - 2S Ícone do Moodle

Active? Yes
Responsible unit: Department of Physics and Astronomy
Course/CS Responsible: Master in Physics

Cycles of Study/Courses

Acronym No. of Students Study Plan Curricular Years Credits UCN Credits ECTS Contact hours Total Time
M:EF 3 Official Study Plan since 2021_M:EF 1 - 6 42 162
M:F 2 Official Study Plan 1 - 6 42 162

Teaching Staff - Responsibilities

Teacher Responsibility
Nuno Miguel Azevedo Silva

Teaching - Hours

Theoretical and practical : 3,23
Type Teacher Classes Hour
Theoretical and practical Totals 1 3,231
Nuno Miguel Azevedo Silva 3,231

Teaching language

English
Obs.: Inglês

Objectives

To give the students an insight into optical sensing, mainly interferometric based, supported by classical, semi-classical and quantum principles, addressing in each of the cases the relevant characteristics, applications, noise sources and signal analysis techniques.

Learning outcomes and competences

The students will be able to understand the basic principles of interferometric optical sensing, including the effect of the source coherence in the sensing device.

They are expected to understand homodyne and heterodyne techniques for signal recovery.

The students should understand the evolution from classical to semi-classic optical sensors, as well as the importance of quantum sensing for ultra-precise measurements.

Working method

Presencial

Program

A. Sensing and data analysis techniques and methods

  • What is a sensor and how to characterize one: limit, ranges, sensitivity, saturation, and noise;
  • Handling experimental data: measurement, errors, and conveying the message with informative graphs;
  • Brief introduction to machine learning techniques and best practices for science: regression and classification.

B. Classical Optical Interferometers for Measurement/Sensing

  • Why Light Excels in sensing and what is an interferometer;
  • The building-blocks of interferometers: optical sources; splitters; polarization control; photodetectors (multiple and single photon detection, and sources of noise);
  • Signal-to-noise ratio and merit factor of an interferometer.
B.1. Homodyne detection
  • What is homodyne detection and how to use it: From fibers to free space;
  • Hands-on with digital off-axis holography for wavefront sensing;
B.2. Heterodyne detection
  • Pros and cons of heterodyne detection for phase recovery in optical interferometers and characterization of their performance;
  • Hands-on with heterodyne detection in the context of optical fiber sensors;
B.3. Outlook and perspectives of classical interferometers
  • Discussion of the past, present and future of interferometers: distributed sensing, distributed acoustic sensing, vernier effect, integrated optics, and optofluidics;

C. Semi-Classical Optical Interferometers for Measurement/Sensing

  • The Heisenberg phase resolution limit in an optical interferometer
  • What is squeezed light and how to generate it using optical non-linear interactions (optical parametric amplification and frequency doubling)
C.1. The case study of the LIGO interferometric observatory

D. Optical Interferometers for Quantum Measurement/Sensing

  • Entangled photons and interferometers.
  • Optical sources for emission of entangled photons and optical detectors with the ability to distinguish photon numbers at the level of single photons.
  • Optical sources for detection of photons, and signal-to-noise ratio.
  • The entangled N00N quantum state in a Mach-Zehnder interferometer.
  • The environment problem.
  • Evolution of the signal processing techniques mastered in classical optical interferometry to address the phase recovery in quantum interferometers.
  • Quantum sensor and the sensing protocol.
D.1. Outlook of Quantum optical sensing
  • Quantum metrology and its future impact: the road to ultra sensitivity, super resolution, and the International System of Units.

E. Additional survey of optical sensors

Mandatory literature

Robert D. Guenther; Modern optics. ISBN: 0-471-51288-5

Complementary Bibliography

Reitze, David; Saulson, Peter; Grote, Hartmut (Editors); Advanced Interferometric Gravitational-wave Detectors: Essentials of Gravitational Wave Detectors. ISBN: 978-9813146075
Bachor, Hans-A.; Ralph, Timothy C.; A Guide to Experiments in Quantum Optics. ISBN: 978-3-527-41193-1
Max Born; Principles of optics. ISBN: 0-08-018018-3

Teaching methods and learning activities

Classes based on interactive discussion of the theoretical concepts, with relevant examples and problem solving.

Hands-on activities and demonstrations (computational and experimental).

Visits to laboratories in order to understand relevant experiments ongoing on the research labs.

Evaluation Type

Distributed evaluation with final exam

Assessment Components

designation Weight (%)
Exame 60,00
Trabalho escrito 40,00
Total: 100,00

Amount of time allocated to each course unit

designation Time (hours)
Estudo autónomo 120,00
Frequência das aulas 42,00
Total: 162,00

Eligibility for exams

According to the FCUP regulations for the assessment of students

Calculation formula of final grade

All students must take the final exam.

Sudents can choose to be assessed only based on the final exam, in which case the exam grade is the final grade.

An optional written report can be considered for 40% of the grade. In this case, the final grade is computed as:

    Final = 0.6×E + 0.4×R (E: exam, R: report)
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