Главная
Study mode:
on
1
Intro
2
Anatomy of a relativistic astrophysical source
3
Connecting the puzzle
4
Astroparticle Physics
5
Neutrinos: probe of deeper horizon, denser environments
6
The MM context of neutrinos
7
Astrophysics with TeV neutrinos
8
km³ detectors
9
The next Generation
10
Future global network of neutrino observatories
11
Detection Principle
12
IceCube Point source sensitivity
13
Phenomenology : Neutrinos
14
High-energy Astrophysical neutrinos
15
PeV neutrinos and Fermi Blazars
16
Neutrino point sources?
17
Hotspot in the Northern sky
18
Current hottest spot
19
Beware of opaque EM sources!
20
Time-dependent searches
21
High-energy neutrino counterparts
22
IceCube 170922A-TXS 0506+056
23
Energetics of the SED
24
MM view of NGC 1068
25
How can CTA contribute?
26
A closer look at the neutrino sky
27
Virtual Observatory Data Tools
28
Most promising results in blazar- neutrino cross-match
Description:
Save Big on Coursera Plus. 7,000+ courses at $160 off. Limited Time Only! Grab it Explore the fascinating world of neutrinos, active galactic nuclei (AGNs), and gamma-rays in this comprehensive lecture from the Latin-American School on CTA Science. Delve into the anatomy of relativistic astrophysical sources and discover how astroparticle physics connects the puzzle pieces. Learn about neutrinos as probes of deeper horizons and denser environments, and understand their role in the multi-messenger context. Examine the principles of km³ detectors and the future global network of neutrino observatories. Investigate high-energy astrophysical neutrinos, including PeV neutrinos and their connection to Fermi Blazars. Analyze neutrino point sources, time-dependent searches, and high-energy neutrino counterparts, with a focus on the IceCube 170922A-TXS 0506+056 event. Explore the energetics of spectral energy distributions and the multi-messenger view of NGC 1068. Discover how the Cherenkov Telescope Array (CTA) can contribute to neutrino studies and gain insights into the most promising results in blazar-neutrino cross-matching using virtual observatory data tools. Read more

Neutrinos, AGNs and Gamma-rays - Class 3

ICTP-SAIFR
Add to list
0:00 / 0:00