Počet záznamů: 1  

Entanglement harvesting for different gravitational wave burst profiles with and without memory

  1. 1.
    SYSNO ASEP0576949
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevEntanglement harvesting for different gravitational wave burst profiles with and without memory
    Tvůrce(i) Barman, S.R. (IN)
    Chakraborty, I. (IN)
    Mukherjee, Sajal (ASU-R)
    Celkový počet autorů3
    Číslo článku180
    Zdroj.dok.Journal of High Energy Physics. - : Springer - ISSN 1029-8479
    Roč. 9, September (2023)
    Poč.str.40 s.
    Forma vydáníOnline - E
    Jazyk dok.eng - angličtina
    Země vyd.DE - Německo
    Klíč. slovaclassical theories of gravity ; thermalfield theory ; high energy physics
    Obor OECDParticles and field physics
    Způsob publikováníOpen access
    Institucionální podporaASU-R - RVO:67985815
    UT WOS001077656900001
    EID SCOPUS85173079294
    DOI10.1007/JHEP09(2023)180
    AnotaceIn the present article, we study how different gravitational wave (GW) burst profiles in linearized gravity, with and without the asymptotic memory, may influence the harvesting between two static Unruh-DeWitt detectors. To this end, we investigate the following burst profiles Gaussian, sech-squared, Heaviside step function, and tanh. Out of these, the first two bursts contain no memory, while the latter two consist of a non-vanishing memory effect. We find that in all of these cases, entanglement harvesting is possible, and it decreases with the increasing distance between detectors and the detector transition energy. We observe that the harvesting differs qualitatively based on the presence or absence of the memory, which is prominent in a low transition energy regime. With memory, the harvesting keeps increasing with decreasing transition energy, while without memory, it tends to reach finite values. Furthermore, for the two burst profiles without memory, longer bursts correspond to greater harvesting in the low detector transition energy regime, and this characteristic is reversed for larger transition energy. Meanwhile, for the tanh-type profile with memory, harvesting is always greater for shorter bursts. We discuss various implications of our findings.
    PracovištěAstronomický ústav
    KontaktRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Rok sběru2024
    Elektronická adresahttps://hdl.handle.net/11104/0346971
Počet záznamů: 1  

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