TEORICAL COSMOLOGY

Course objectives

GENERAL OBJECTIVES: The course aims to teach the student mainly the theory of structures formation, both in the early stages of linear evolution and in the most advanced phases. At the same time, statistical methods will be analyzed to compare theoretical predictions with observational data. Finally, the student will learn the main elements of gravitational lensing, both the theoretical aspects and its use in astrophysics and cosmology SPECIFIC OBJECTIVES: A - Knowledge and understanding OF 1) To know the equations that regulate the growth of density perturbations in different cosmological scenarios OF 2) To understand the role of the radiative, baryonic and dark matter components in the formation of cosmic structures OF 3) To know the statistical properties of Gaussian stochastic fields and in particular those of the perturbation power spectrum OF 4) To know the spherical collapse model and the role of numerical simulations in cosmology OF 5) To know the statistical methods used in the analysis of collapsed objects OF 6) To know the equations that determine the deflection of light by massive objects, in particular those concerning the formation of multiple images and the distortion of background sources … B - Application skills OF 7) To be able to deduce the properties of the large-scale structure of the Universe as a function of the different dynamic components and different types of primordial spectrum OF 8) To be able to apply statistical methods to data analysis of different cosmological probes OF 9) To be able to deduce the properties of collapsed structures from those of the density field in linear regime using the Press-Schechter formalism OF 10) To be able to apply the lensing equations in the case of the main astrophysical and cosmological applications C - Autonomy of judgment OF 11) To be able to integrate the concepts acquired in order to apply them in the more general context of cosmology and extra-galactic astrophysics D - Communication skills OF 12) To know how to communicate concepts and ideas in the cosmology field with an appropriate mathematical language and formalism E - Ability to learn OF 13) Have the ability to read scientific papers in order to further explore some of the topics introduced during the course

Channel 1
ROBERTO MAOLI Lecturers' profile

Program - Frequency - Exams

Course program
LINEAR EVOLUTION OF PERTURBATIONS: Gravitational instability in a static or expanding universe –Jeans mass and dissipation mass – Perturbations growth in general relativity. STATISTICAL METHODS FOR THE STUDY OF THE DENSITY FIELD: Introduction to statistical methods: stochastic and gaussian fields, correlation function, Wiener-Khintchine theorem, convolution, mass variance – Perturbation spectrum: scale-free and Harrison-Zel’dovich spectra, spectrum by inflation, transfer function. NON-LINEAR EVOLUTION OF PERTURBATIONS: Spherical collapse and Zel’dovich approximation – N-body simulations – Galaxy formation. STATISTICAL METHODS FOR THE STUDY OF FORMED STRUCTURES: Clustering properties of the universe: two points and angular correlation functions, Limber equation, percolation, bias factor – Mass function: Press-Schechter approach, excursion sets approach. GRAVITATIONAL LENSING: General concepts: Shapiro delay, lens equation, lensing potential, convergence and shear fields, multiple images – Cosmological applications: microlensing, Hubble constant measurements, cluster mass reconstruction, CMB lensing, cosmic shear.
Prerequisites
The course has not prerequisites but the attendency of Physical Cosmology course is suggested.
Books
G. Tormen – Formazione delle Strutture Cosmiche - Lecture notes - cap. 1-6, 10 P. Coles & F. Lucchin – Cosmology: origin and evolution of cosmic structure – Ed.Wiley & Sons - cap. 7, 10-16 T. Padmanabhan – Structure formation in the universe – Cambridge Univ. Press - cap. 8 N. Vittorio – Cosmology – Series in Astronomy and Astrophysics – CRC Press H Mo, F. van den Bosch & S. White – Galaxy Formation and Evolution – Cambridge Univ. Press - cap. 1.4, 15.7, ann. C M. Meneghetti–Introduction to Gravitational Lensing - Lecture notes - cap. 1-2
Teaching mode
The lecture format is through blackboard and slide presentation (mostly for the part of the course on N-body simulation, galaxy formation and gravitational lensing).
Frequency
The attendance of lessons is not mandatory but it is strongly recommended.
Exam mode
The evaluation is based on an oral interview of about one hour.
Lesson mode
The lecture format is through blackboard and slide presentation (mostly for the part of the course on N-body simulation, galaxy formation and gravitational lensing).
  • Lesson code1012136
  • Academic year2025/2026
  • CourseAstrophysics and Cosmology
  • CurriculumSingle curriculum
  • Year2nd year
  • Semester1st semester
  • SSDFIS/05
  • CFU6