Difference between revisions of "Fundamental Physics Working Group"
Micheledoro (talk | contribs) (→LIV searches at BL LAC) |
Micheledoro (talk | contribs) (→DM searches at the GC) |
||
| Line 29: | Line 29: | ||
=== DM searches at the GC === | === DM searches at the GC === | ||
| − | + | * PI: M. Huetten. Team: M. Doro | |
| − | + | * Abstract: | |
| − | ** | + | * Project webpage: |
=== ALP searches on Mrk 421 === | === ALP searches on Mrk 421 === | ||
Revision as of 08:40, 27 May 2022
Back to Main page
Back to Data Analysis
The Fundamental Physics Science Group focuses on the analysis of fundamental physics that can be done with LST-1 data, such as dark matter, Lorentz Invariance, Rare event search, and cosmic-ray physics.
Contents
Members
Join us! Mailing list: join here Current Coordinators: Michele Doro (Leader) [1], Moritz Hütten (Deputy) Past Coordinators: NA
Meetings and Minutes
Indico starting page (Meetings, Slides, and minutes): https://indico.cta-observatory.org/category/172/
- WG meeting: 2022/03/22 [2]. Minutes: File:LST1 FUND PHYS minutes 22 03 2022.pdf
- WG meeting: 2022/04/19 [3]. Focus on Cosmic Ray Searches. Minutes File:LST1 FUND PHYS minutes 19 04 2022.pdf
- WG meeting: 2022/05/24 [4]. Focus on LIV searches. Minutes File:LST1 FUND PHYS minutes 24 05 2022.pdf
- WG meeting: 2022/06/21 [5]. Focus on DM
- WG meeting: 2022/07/19 Focus on ALP
Projects in progress:
In the following we add a list of projects, more or less ordered by advancement and importance. Please add your name if interested.
LIV searches at BL LAC
- PI: Sami. * Team:
- Abstract:
- Project webpage
DM searches at the GC
- PI: M. Huetten. Team: M. Doro
- Abstract:
- Project webpage:
ALP searches on Mrk 421
- PI: I. Batkovic [6]. Team: G. D'Amico, M. Doro, M. Manganaro. Contact us if interested
- Abstract: Axion Like Particles can be detected as wiggles in the spectra of faraway targets whose high energy emission crossed intense and ample region of magnetic fields. Such targets are the high energy emission from galaxies in Galaxy Cluster's core or those emitted within relativistic jets. Here we focus on the second class, and in particular on Mrk421 jet. The investigation relies on the modelization of the B-field in the ultrarelativistic jet.
- Project webpage: TBD
Direct Cherenkov
- PI: Seiya Nozaki. Team: D. Paneque, G. Fernandez, M. Doro, Ohtani, D. Della Volpe, R. Lopez Coto, F. Cassol, G. Emery, Ohishi, P. Bordas,
- Abstract:
- Link: Project Webpage
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
Useful Tools
- Observability display https://airmass.org/chart/obsid:lapalma/
- Coordinate converter http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/convcoord/convcoord.pl
- Distance converter http://www.convertworld.com/en/length/Parsec.html
- Energy/frequency/wavelength converter http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/energyconv/energyConv.pl
- A Date/Time Conversion Utility http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/xTime/xTime.pl
- Flux/count rate converter http://heasarc.gsfc.nasa.gov/Tools/w3pimms.html
- Catalog of TeV source http://tevcat.uchicago.edu/
- Publication of HESS, MAGIC and VERITAS
- To calculate source observability (you may have to introduce LST-1 coordinates 28.76195, -17.89005) http://www.magic.iac.es/scheduler/ or https://www.mpi-hd.mpg.de/hfm/HESS/public/Visibility.html
