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

The result's identifiers

  • Result code in 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>

  • Result on the web

    <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>

Alternative languages

  • Result language

    angličtina

  • Original language name

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

  • Original language description

    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.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10306 - Optics (including laser optics and quantum optics)

Result continuities

  • Project

    <a href="/en/project/EH23_021%2F0008790" target="_blank" >EH23_021/0008790: Optical technologies</a><br>

  • Continuities

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

Others

  • Publication year

    2025

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    PHYSICAL REVIEW A

  • ISSN

    2469-9926

  • e-ISSN

    2469-9934

  • Volume of the periodical

    112

  • Issue of the periodical within the volume

    6

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    11

  • Pages from-to

    "063712-1"-"063712-11"

  • UT code for WoS article

    001641472900002

  • EID of the result in the Scopus database

    2-s2.0-105027527598