Fundamental Physics Working Group
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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.
Current Coordinators: Michele Doro (Leader) [1], Moritz Hütten (Deputy)
Past Coordinators: NA
Contents
Meetings and Minutes
Indico page (Meetings, Slides, and minutes): https://indico.cta-observatory.org/category/172/
- 1st LST1 PHYS FUND WG meeting: 2022/03/22 [2]. Minutes: File:LST1 FUND PHYS minutes 22 03 2022.pdf
- 2nd LST1 PHYS FUND WG meeting: 2022/04/19 [3]. Focus on Cosmic Ray Searches. Minutes File:LST1 FUND PHYS minutes 19 04 2022.pdf
- 3rd LST1 PHYS FUND WG meeting: 2022/05/24 [4]. Focus on LIV searches. Minutes File:LST1 FUND PHYS minutes 24 05 2022.pdf
- 4th LST1 PHYS FUND WG meeting: 2022/06/21 [5]. Focus on DM
- 5th LST1 PHYS FUND WG meeting: 2022/07/19 Focus on ALP
Members
Join us! Mailing list: join here
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
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:
- DM searches at the GC
- PI: M. Huetten
- Team: M. Doro
- Abstract:
- ALP searches on Mrk 421
- PI: I. Batkovic
- Team: G. D'Amico, M. Doro, M. Manganaro
- Abstract:
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