Difference between revisions of "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.''' | '''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.''' | ||
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| + | ===Members=== | ||
| + | '''Join us!''' Mailing list: [https://portal.cta-observatory.org/_layouts/people.aspx?MembershipGroupId=3843 join here] | ||
'''Current Coordinators''': Michele Doro (Leader) [mailto:michele.doro@unipd.it], Moritz Hütten (Deputy) | '''Current Coordinators''': Michele Doro (Leader) [mailto:michele.doro@unipd.it], Moritz Hütten (Deputy) | ||
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'''Past Coordinators''': NA | '''Past Coordinators''': NA | ||
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=== Meetings and Minutes=== | === Meetings and Minutes=== | ||
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* 5th LST1 PHYS FUND WG meeting: 2022/07/19 Focus on ALP | * 5th LST1 PHYS FUND WG meeting: 2022/07/19 Focus on ALP | ||
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== Projects in progress: == | == 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. | 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 | ** PI: Sami | ||
** Team: | ** Team: | ||
** Abstract: | ** Abstract: | ||
| − | + | ||
| + | === DM searches at the GC === | ||
** PI: M. Huetten | ** PI: M. Huetten | ||
** Team: M. Doro | ** Team: M. Doro | ||
** Abstract: | ** Abstract: | ||
| − | + | ||
| − | + | === ALP searches on Mrk 421 === | |
| − | + | * PI: I. Batkovic [mailto:ivana.batkovic@phd.unipd.it] | |
| − | + | * 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. | ||
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| + | == Papers in advanced stage: == | ||
| + | === Published / Accepted === | ||
| + | === Resubmitted === | ||
| + | === Submitted === | ||
| + | === Nearing submission (internal review) === | ||
==Useful Tools== | ==Useful Tools== | ||
Revision as of 08:08, 27 May 2022
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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.
Contents
Members
Join us! Mailing list: join here Current Coordinators: Michele Doro (Leader) [1], Moritz Hütten (Deputy) Past Coordinators: NA
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
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 [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.
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
