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- Experimental Cosmology
- Summary
Insegnamento
Course full name
Experimental Cosmology
Course ID number
2122-1-F5802Q009
Course Syllabus
Aims
Knowledge of observational evidences and experimental techniques for cosmology.
Contents
Elements of cosmology. Cosmic Microwave Background: history and current status of measurements. The sky at millimeter and submillimeter wavelengths. Physical observables, cosmological parameters and experimental techniques.
Detailed program
• Historical recalls, short review on modern cosmology
• Observational evidence supporting the Big Bang
• Late time observational probes
• Cosmic Microwave background
◦ CMB history, spectrum, primary anisotropies
◦ CMB polarization
◦ Primordial gravitational waves and inflation
◦ CMB statistics
• CMB Foregrounds
◦ Galactic synchrotron
◦ Free free
◦ Dust (thermal, spinning, grain alignment...), hints on star formation
◦ Point sources (Radio and IR galaxies)
• Observing the microwave sky
◦ Telescopes: current status, different designs, ground, balloon and satellites
◦ Detectors: bolometers, TES, KIDs
◦ Receivers: cryostats, filters, cold optics, lenses, horns,
◦ Experimental techniques: readout, modulators, signal processing, polarimetry
◦ Instrument characterization and calibration
• From CMB maps to cosmological parameters
• Large Scale Structure Observations
◦ Galaxies as probes of the cosmic density field
◦ Gravitational lensing and Cosmic shear, CMB lensing
◦ Galaxy clusters as probes for cosmology, SZ effect
• Cosmic dark ages
◦ Cosmic reionization
◦ Hints on Cosmic star formation history, high redshift galaxies
• Observational evidence supporting the Big Bang
• Late time observational probes
• Cosmic Microwave background
◦ CMB history, spectrum, primary anisotropies
◦ CMB polarization
◦ Primordial gravitational waves and inflation
◦ CMB statistics
• CMB Foregrounds
◦ Galactic synchrotron
◦ Free free
◦ Dust (thermal, spinning, grain alignment...), hints on star formation
◦ Point sources (Radio and IR galaxies)
• Observing the microwave sky
◦ Telescopes: current status, different designs, ground, balloon and satellites
◦ Detectors: bolometers, TES, KIDs
◦ Receivers: cryostats, filters, cold optics, lenses, horns,
◦ Experimental techniques: readout, modulators, signal processing, polarimetry
◦ Instrument characterization and calibration
• From CMB maps to cosmological parameters
• Large Scale Structure Observations
◦ Galaxies as probes of the cosmic density field
◦ Gravitational lensing and Cosmic shear, CMB lensing
◦ Galaxy clusters as probes for cosmology, SZ effect
• Cosmic dark ages
◦ Cosmic reionization
◦ Hints on Cosmic star formation history, high redshift galaxies
Teaching form
2 CFU, frontal teaching, biweekly lectures in English
Textbook and teaching resource
Course slides and notes
B. Ryden, Introduction to Cosmology
S. Serjeant, Observational Cosmology
Articles indicated during lectures
Semester
Second semester
Assessment method
Oral exam (presentation + open questions)
Office hours
Tue. 9:00-10:00 or by appointment
Key information
Field of research
FIS/05
ECTS
6
Term
Second semester
Activity type
Mandatory to be chosen
Course Length (Hours)
42
Staff
-
Federico Nati