| Title: | Multi-messenger study with the Pierre Auger Observatory |
|---|
| Authors: | ID Yang, Lili, University of Nova Gorica (Author) |
|---|
| Files: |
This document has no files that are freely available to the public. This document may have a physical copy in the library of the organization, check the status via COBISS.  |
|---|
| Language: | English |
|---|
| Work type: | Not categorized |
|---|
| Typology: | 3.16 - Unpublished Invited Conference Lecture |
|---|
| Organization: | UNG - University of Nova Gorica
|
|---|
| Abstract: | The Pierre Auger Observatory is the largest cosmic ray detector in the world, studying particles with energy above 10^17 eV. Even though Auger is dedicated to charged cosmic rays, it’s also sensitive to ultra-high energy neutral particles, such as photons, neutrinos and neutrons, which are undeflected by magnetic field and pointing back to the source site. More exciting, with the breakthrough observations of gravitational-wave signal, the new era of multi-messenger analysis has come. I will present the recent results and prospects of multi-messenger study with Auger and also the first joint detection of gravitational and electromagnetic radiation from the source, with a focus on the UHE neutrino search. |
|---|
| Keywords: | Pierre Auger Observatory, multi-messenger, neutrino, gravitational wave |
|---|
| Place of performance: | Shanghai, China |
|---|
| Year of performance: | 2017 |
|---|
| PID: | 20.500.12556/RUNG-3540-d53f60e3-26ea-affb-aa5c-e757294cc55c |
|---|
| COBISS.SI-ID: | 4989691 |
|---|
| NUK URN: | URN:SI:UNG:REP:SUSPZ9ST |
|---|
| Publication date in RUNG: | 17.01.2018 |
|---|
| Views: | 3982 |
|---|
| Downloads: | 0 |
|---|
| Metadata: |     |
|---|
|
:
|
Copy citation |
|---|
| | | | Average score: | (0 votes) |
|---|
| Your score: | Voting is allowed only for logged in users. |
|---|
| Share: |  |
|---|
Hover the mouse pointer over a document title to show the abstract or click
on the title to get all document metadata. |
