Code: | AST4008 | Acronym: | AST4008 |
Keywords | |
---|---|
Classification | Keyword |
OFICIAL | Astronomy |
Active? | Yes |
Responsible unit: | Department of Physics and Astronomy |
Course/CS Responsible: | Master in Astronomy and Astrophysics |
Acronym | No. of Students | Study Plan | Curricular Years | Credits UCN | Credits ECTS | Contact hours | Total Time |
---|---|---|---|---|---|---|---|
M:A_ASTR | 7 | Study plan since academic year 2024/2025 | 1 | - | 6 | 42 | 162 |
2 | |||||||
M:F | 10 | Official Study Plan | 1 | - | 6 | 42 | 162 |
Teacher | Responsibility |
---|---|
Orfeu Bertolami Neto |
Theoretical and practical : | 3,23 |
Type | Teacher | Classes | Hour |
---|---|---|---|
Theoretical and practical | Totals | 1 | 3,231 |
Orfeu Bertolami Neto | 3,231 |
The overall objective of this lecture course is to develop in the students an interest in cosmology, communicating to them in a consistent fashion the basic principles as well as the latest developments in this area.
After the frequency of this lecture course, students should be able to: understand the fundamental assumptions behind the standard cosmological model; deduce the equations that describe the dynamics of the Universe; describe the observational evidence of the standard cosmological model; understand the successes and limitations of the standard cosmological model; understand the thermodynamic processes most relevant in cosmology, in particular recombination and primordial nucleosynthesis; describe the observational constraints on cosmological parameters and their consequences for the evolution of the Universe; understand the relevance of scalar fields in cosmology, particularly in solving some of the problems of the standard cosmological model; understand the linear and nonlinear evolution of fluctuations in the density of matter in different eras and scales; understand the mechanisms responsible for the anisotropy of the cosmic microwave background and its relation to the large-scale structure of Universe; describe the observational evidence for dark matter and dark energy. This course also aims to develop a wide range of complementary skills in various areas, such as personal and inter-personal organization, written and oral communication, culture in physics and astronomy and the search and selection of bibliography.
1. Introduction
1.1 Basic concepts in Astronomy
1.2 Relevant observations for Cosmology
2. The expanding Universe
2.1 The cosmological principle
2.2 The Robertson-Walker metric
2.3 The cosmological redshift
2.4 Peculiar velocities
2.5 Equation of state
3. Relativistic cosmology
3.1 Friedmann equation: deduction and solutions
3.2 Cosmological horizons and the age of the Universe
3.3 Angular and luminosity cosmological distances
4. The primordial Universe
4.1 Cronology
4.2 Particles in thermal equilibrium
4.3 Entropy
4.4 Decoupling of relativistic and non-relativistic particles
4.5 Primordial nucleosynthesis
4.6 The cosmic microwave background
5. Inflation
5.1 Problems in the standard cosmological model
5.2 Inflationary models
In the lecture classes the contents in the program are taught and their application clarified through examples.
designation | Weight (%) |
---|---|
Exame | 80,00 |
Trabalho prático ou de projeto | 20,00 |
Total: | 100,00 |
designation | Time (hours) |
---|---|
Frequência das aulas | 42,00 |
Estudo autónomo | 120,00 |
Total: | 162,00 |
The assessment for the Cosmology course consists of a final exam and the resolution of problems. The final classification in this course will be equal to the classification obtained in the final exam plus up to 4 points due to the resolution of problems. To be successful the students must obtain at least 8 points in the grading of the exam.