20410506 - COSMOLOGY

The aim of the course is to critically discuss the most relevant issues - some of them still open - concerning Modern Cosmology. We will illustrate its state-of-the-art, and the methods - both theoretical and observational - currently used to investigate its properties. We will further provide a coherent vision which starts from the Big Bang and arrives to the formation of the first galaxies. 

Curriculum

teacher profile | teaching materials

Fruizione: 20402143 COSMOLOGIA in Fisica LM-17 R N0 MAGLIOCCHETTI Manuela

Programme

60 hours of lectures

• Brief review of general relativity and Einstein's equation

• Robertson-Walker metric

• Hubble's law and Hubble tension

• Redshift

• Cosmological distances

• The cosmological constant

• Friedmann and Einstein-de Sitter models

• Thermal history of the Universe

• Cosmic Microwave Background (CMB)

• Jeans theory for gravitational instability

• Application of Jeans theory in cosmology: linear evolution

• Structure Formation I: baryon-only case

• Structure Formation II: case including non-baryonic matter
•Spettro delle perturbazioni, filtri e funzioni di trasferimento

• Spectrum of perturbations, filters, and transfer functions

• Covariance functions

• Theory and observations related to linear theory: CMB fluctuations

• Non-linear evolution of perturbations

• Large-scale structure of the Universe: statistical analysis of galaxy distribution

• Virialized structures: Press and Schechter theory and its extension

• Luminous matter and dark matter: the bias problem

• Brief overview of current and future cosmological missions: Euclid

• Brief overview of extragalactic radio sources

Completion of 64 hours: study of the article

"Hosts and Environments: a (large-scale) radio history of AGN and star-forming galaxies"

(https://link.springer.com/article/10.1007/s00159-022-00142-1)

Core Documentation

Testi principali:

- Cosmology: The Origin and Evolution of Cosmic Structure by P. Coles and F. Lucchin

- Structure Formation in the Universe by T. Padhmanaban



Testi consigliati:

- Cosmological Physics by J.A. Peacock

- The Large Scale Structure of the Universe by P.J.E. Peebles

Attendance

Attendance isn't mandatory, but it's always highly recommended

Type of evaluation

The exam will consist of discussing a chapter of your choice from the above-mentioned article and then continue with questions on the entire program covered in class.

teacher profile | teaching materials

Fruizione: 20402143 COSMOLOGIA in Fisica LM-17 R N0 MAGLIOCCHETTI Manuela

Programme

60 hours of lectures

• Brief review of general relativity and Einstein's equation

• Robertson-Walker metric

• Hubble's law and Hubble tension

• Redshift

• Cosmological distances

• The cosmological constant

• Friedmann and Einstein-de Sitter models

• Thermal history of the Universe

• Cosmic Microwave Background (CMB)

• Jeans theory for gravitational instability

• Application of Jeans theory in cosmology: linear evolution

• Structure Formation I: baryon-only case

• Structure Formation II: case including non-baryonic matter
•Spettro delle perturbazioni, filtri e funzioni di trasferimento

• Spectrum of perturbations, filters, and transfer functions

• Covariance functions

• Theory and observations related to linear theory: CMB fluctuations

• Non-linear evolution of perturbations

• Large-scale structure of the Universe: statistical analysis of galaxy distribution

• Virialized structures: Press and Schechter theory and its extension

• Luminous matter and dark matter: the bias problem

• Brief overview of current and future cosmological missions: Euclid

• Brief overview of extragalactic radio sources

Completion of 64 hours: study of the article

"Hosts and Environments: a (large-scale) radio history of AGN and star-forming galaxies"

(https://link.springer.com/article/10.1007/s00159-022-00142-1)

Core Documentation

Testi principali:

- Cosmology: The Origin and Evolution of Cosmic Structure by P. Coles and F. Lucchin

- Structure Formation in the Universe by T. Padhmanaban



Testi consigliati:

- Cosmological Physics by J.A. Peacock

- The Large Scale Structure of the Universe by P.J.E. Peebles

Attendance

Attendance isn't mandatory, but it's always highly recommended

Type of evaluation

The exam will consist of discussing a chapter of your choice from the above-mentioned article and then continue with questions on the entire program covered in class.

teacher profile | teaching materials

Fruizione: 20402143 COSMOLOGIA in Fisica LM-17 R N0 MAGLIOCCHETTI Manuela

Programme

60 hours of lectures

• Brief review of general relativity and Einstein's equation

• Robertson-Walker metric

• Hubble's law and Hubble tension

• Redshift

• Cosmological distances

• The cosmological constant

• Friedmann and Einstein-de Sitter models

• Thermal history of the Universe

• Cosmic Microwave Background (CMB)

• Jeans theory for gravitational instability

• Application of Jeans theory in cosmology: linear evolution

• Structure Formation I: baryon-only case

• Structure Formation II: case including non-baryonic matter
•Spettro delle perturbazioni, filtri e funzioni di trasferimento

• Spectrum of perturbations, filters, and transfer functions

• Covariance functions

• Theory and observations related to linear theory: CMB fluctuations

• Non-linear evolution of perturbations

• Large-scale structure of the Universe: statistical analysis of galaxy distribution

• Virialized structures: Press and Schechter theory and its extension

• Luminous matter and dark matter: the bias problem

• Brief overview of current and future cosmological missions: Euclid

• Brief overview of extragalactic radio sources

Completion of 64 hours: study of the article

"Hosts and Environments: a (large-scale) radio history of AGN and star-forming galaxies"

(https://link.springer.com/article/10.1007/s00159-022-00142-1)

Core Documentation

Testi principali:

- Cosmology: The Origin and Evolution of Cosmic Structure by P. Coles and F. Lucchin

- Structure Formation in the Universe by T. Padhmanaban



Testi consigliati:

- Cosmological Physics by J.A. Peacock

- The Large Scale Structure of the Universe by P.J.E. Peebles

Attendance

Attendance isn't mandatory, but it's always highly recommended

Type of evaluation

The exam will consist of discussing a chapter of your choice from the above-mentioned article and then continue with questions on the entire program covered in class.

teacher profile | teaching materials

Fruizione: 20402143 COSMOLOGIA in Fisica LM-17 R N0 MAGLIOCCHETTI Manuela

Programme

60 hours of lectures

• Brief review of general relativity and Einstein's equation

• Robertson-Walker metric

• Hubble's law and Hubble tension

• Redshift

• Cosmological distances

• The cosmological constant

• Friedmann and Einstein-de Sitter models

• Thermal history of the Universe

• Cosmic Microwave Background (CMB)

• Jeans theory for gravitational instability

• Application of Jeans theory in cosmology: linear evolution

• Structure Formation I: baryon-only case

• Structure Formation II: case including non-baryonic matter
•Spettro delle perturbazioni, filtri e funzioni di trasferimento

• Spectrum of perturbations, filters, and transfer functions

• Covariance functions

• Theory and observations related to linear theory: CMB fluctuations

• Non-linear evolution of perturbations

• Large-scale structure of the Universe: statistical analysis of galaxy distribution

• Virialized structures: Press and Schechter theory and its extension

• Luminous matter and dark matter: the bias problem

• Brief overview of current and future cosmological missions: Euclid

• Brief overview of extragalactic radio sources

Completion of 64 hours: study of the article

"Hosts and Environments: a (large-scale) radio history of AGN and star-forming galaxies"

(https://link.springer.com/article/10.1007/s00159-022-00142-1)

Core Documentation

Testi principali:

- Cosmology: The Origin and Evolution of Cosmic Structure by P. Coles and F. Lucchin

- Structure Formation in the Universe by T. Padhmanaban



Testi consigliati:

- Cosmological Physics by J.A. Peacock

- The Large Scale Structure of the Universe by P.J.E. Peebles

Attendance

Attendance isn't mandatory, but it's always highly recommended

Type of evaluation

The exam will consist of discussing a chapter of your choice from the above-mentioned article and then continue with questions on the entire program covered in class.

teacher profile | teaching materials

Fruizione: 20402143 COSMOLOGIA in Fisica LM-17 R N0 MAGLIOCCHETTI Manuela

Programme

60 hours of lectures

• Brief review of general relativity and Einstein's equation

• Robertson-Walker metric

• Hubble's law and Hubble tension

• Redshift

• Cosmological distances

• The cosmological constant

• Friedmann and Einstein-de Sitter models

• Thermal history of the Universe

• Cosmic Microwave Background (CMB)

• Jeans theory for gravitational instability

• Application of Jeans theory in cosmology: linear evolution

• Structure Formation I: baryon-only case

• Structure Formation II: case including non-baryonic matter
•Spettro delle perturbazioni, filtri e funzioni di trasferimento

• Spectrum of perturbations, filters, and transfer functions

• Covariance functions

• Theory and observations related to linear theory: CMB fluctuations

• Non-linear evolution of perturbations

• Large-scale structure of the Universe: statistical analysis of galaxy distribution

• Virialized structures: Press and Schechter theory and its extension

• Luminous matter and dark matter: the bias problem

• Brief overview of current and future cosmological missions: Euclid

• Brief overview of extragalactic radio sources

Completion of 64 hours: study of the article

"Hosts and Environments: a (large-scale) radio history of AGN and star-forming galaxies"

(https://link.springer.com/article/10.1007/s00159-022-00142-1)

Core Documentation

Testi principali:

- Cosmology: The Origin and Evolution of Cosmic Structure by P. Coles and F. Lucchin

- Structure Formation in the Universe by T. Padhmanaban



Testi consigliati:

- Cosmological Physics by J.A. Peacock

- The Large Scale Structure of the Universe by P.J.E. Peebles

Attendance

Attendance isn't mandatory, but it's always highly recommended

Type of evaluation

The exam will consist of discussing a chapter of your choice from the above-mentioned article and then continue with questions on the entire program covered in class.