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Lorentz invariance violation search with the Cherenkov Telescope Array Observatory Large-Sized Telescope

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F25%3A00646049" target="_blank" >RIV/67985815:_____/25:00646049 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378271:_____/25:00646049 RIV/61989592:15310/25:73635274

  • Result on the web

    <a href="https://pos.sissa.it/501/808/pdf" target="_blank" >https://pos.sissa.it/501/808/pdf</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.501.0808" target="_blank" >10.22323/1.501.0808</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Lorentz invariance violation search with the Cherenkov Telescope Array Observatory Large-Sized Telescope

  • Original language description

    The fast variability of very-high energy (VHE) sources such as pulsars, gamma rays bursts (GRBs) or flares of active galactic nuclei (AGN) can be used to detect or constrain Lorentz invariance violation (LIV) by measuring lags in the arrival time of VHE photons. However, an important source of uncertainty arises from processes within the source that may induce intrinsic photon delays. Combining observations of different sources allows us to probe higher energy scales when LIV effects become relevant as well as to distinguish LIV-induced lags from intrinsic effects. We present the results of a standardized analysis performed on all AGN observations carried out by the first Large-Sized Telescope (LST-1) of CTAO. This analysis includes a general search of intra-night variability in archive observing nights that show significant excesses for the target candidates. The observing nights selected for LIV searches are then combined together to extract limits to the characteristic energies at which the LIV effect is expected to be significant. Finally, similar analysis have been performed on relevant data from other major imaging atmospheric Cherenkov telescopes, H.E.S.S., MAGIC and VERITAS, in order to combine all the data sets to extract combined limits that constrain one of the LIV effects.n

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Proceedings of Science

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

  • Number of pages

    10

  • Pages from-to

    808

  • Publisher name

    Sissa Medilab srl

  • Place of publication

    Trieste

  • Event location

    Ženeva

  • Event date

    Jul 15, 2025

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article