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Certification of stellar ranks of quantum states of light with a pair of click detectors

Identifikátory výsledku

  • Kód výsledku v IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61989592%3A15310%2F25%3A73632915" target="_blank" >RIV/61989592:15310/25:73632915 - isvavai.cz</a>

  • Výsledek na webu

    <a href="https://journals.aps.org/pra/pdf/10.1103/hct3-6hgn" target="_blank" >https://journals.aps.org/pra/pdf/10.1103/hct3-6hgn</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/hct3-6hgn" target="_blank" >10.1103/hct3-6hgn</a>

Alternativní jazyky

  • Jazyk výsledku

    angličtina

  • Název v původním jazyce

    Certification of stellar ranks of quantum states of light with a pair of click detectors

  • Popis výsledku v původním jazyce

    Stellar rank of quantum state of light quantifies the amount of non-Gaussian resources required for its generation. One popular and practical approach to certification of stellar rank is based on measurement of click statistics with an array of binary detectors that can only distinguish the presence and absence of photons. Specifically, it was shown that measurements with an array of 𝑚+1 detectors allow one to certify stellar rank 𝑚 of approximate Fock state |𝑚⟩ , even when the state is subjected to losses or certain noise. Here we address the question as to how many click detectors are in principle required to certify stellar ranks higher than one. We show that two click detectors arranged in a Hanbury Brown-Twiss setup suffice. Interestingly, detection of stellar ranks higher than one is greatly facilitated by making the total detection efficiency of the detectors sufficiently low but well calibrated. Losses affect the response of the detection scheme in a way that can be exploited to certify stellar rank of higher Fock states. We explicitly construct the corresponding stellar rank witnesses and discuss dependence of the stellar rank thresholds on parameters of the considered setup. Our results reveal that it is possible to certify stellar ranks higher than 1 even with a minimalistic scheme that provides only very coarse-grained information about the photon number statistics of the characterized state.

  • Název v anglickém jazyce

    Certification of stellar ranks of quantum states of light with a pair of click detectors

  • Popis výsledku anglicky

    Stellar rank of quantum state of light quantifies the amount of non-Gaussian resources required for its generation. One popular and practical approach to certification of stellar rank is based on measurement of click statistics with an array of binary detectors that can only distinguish the presence and absence of photons. Specifically, it was shown that measurements with an array of 𝑚+1 detectors allow one to certify stellar rank 𝑚 of approximate Fock state |𝑚⟩ , even when the state is subjected to losses or certain noise. Here we address the question as to how many click detectors are in principle required to certify stellar ranks higher than one. We show that two click detectors arranged in a Hanbury Brown-Twiss setup suffice. Interestingly, detection of stellar ranks higher than one is greatly facilitated by making the total detection efficiency of the detectors sufficiently low but well calibrated. Losses affect the response of the detection scheme in a way that can be exploited to certify stellar rank of higher Fock states. We explicitly construct the corresponding stellar rank witnesses and discuss dependence of the stellar rank thresholds on parameters of the considered setup. Our results reveal that it is possible to certify stellar ranks higher than 1 even with a minimalistic scheme that provides only very coarse-grained information about the photon number statistics of the characterized state.

Klasifikace

  • Druh

    J<sub>imp</sub> - Článek v periodiku v databázi Web of Science

  • CEP obor

  • OECD FORD obor

    10306 - Optics (including laser optics and quantum optics)

Návaznosti výsledku

  • Projekt

    <a href="/cs/project/EH23_021%2F0008790" target="_blank" >EH23_021/0008790: Optické technologie</a><br>

  • Návaznosti

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Ostatní

  • Rok uplatnění

    2025

  • Kód důvěrnosti údajů

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

Údaje specifické pro druh výsledku

  • Název periodika

    PHYSICAL REVIEW A

  • ISSN

    2469-9926

  • e-ISSN

    2469-9934

  • Svazek periodika

    112

  • Číslo periodika v rámci svazku

    6

  • Stát vydavatele periodika

    US - Spojené státy americké

  • Počet stran výsledku

    11

  • Strana od-do

    "063712-1"-"063712-11"

  • Kód UT WoS článku

    001641472900002

  • EID výsledku v databázi Scopus

    2-s2.0-105027527598