8,714 research outputs found

    CMB statistical isotropy confirmation at all scales using multipole vectors

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    We present an efficient numerical code and conduct, for the first time, a null and model-independent CMB test of statistical isotropy using Multipole Vectors (MVs) at all scales. Because MVs are insensitive to the angular power spectrum Cβ„“C_\ell, our results are independent from the assumed cosmological model. We avoid a posteriori choices and use pre-defined ranges of scales β„“βˆˆ[2,30]\ell\in[2,30], β„“βˆˆ[2,600]\ell\in[2,600] and β„“βˆˆ[2,1500]\ell\in[2,1500] in our analyses. We find that all four masked Planck maps, from both 2015 and 2018 releases, are in agreement with statistical isotropy for β„“βˆˆ[2,30]\ell\in[2,30], β„“βˆˆ[2,600]\ell\in[2,600]. For β„“βˆˆ[2,1500]\ell\in[2,1500] we detect anisotropies but this is indicative of simply the anisotropy in the noise: there is no anisotropy for β„“<1300\ell < 1300 and an increasing level of anisotropy at higher multipoles. Our findings of no large-scale anisotropies seem to be a consequence of avoiding \emph{a posteriori} statistics. We also find that the degree of anisotropy in the full sky (i.e. unmasked) maps vary enormously (between less than 5 and over 1000 standard deviations) among the different mapmaking procedures and data releases.Comment: v4: additional analysis which increased statistical sensitivity, including new plots and tables; extended discussion; 15 pages, 14 figures, 7 tables. Matches published versio

    The Unruh Quantum Otto Engine

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    We introduce a quantum heat engine performing an Otto cycle by using the thermal properties of the quantum vacuum. Since Hawking and Unruh, it has been established that the vacuum space, either near a black hole or for an accelerated observer, behaves as a bath of thermal radiation. In this work, we present a fully quantum Otto cycle, which relies on the Unruh effect for a single quantum bit (qubit) in contact with quantum vacuum fluctuations. By using the notions of quantum thermodynamics and perturbation theory we obtain that the quantum vacuum can exchange heat and produce work on the qubit. Moreover, we obtain the efficiency and derive the conditions to have both a thermodynamic and a kinematic cycle in terms of the initial populations of the excited state, which define a range of allowed accelerations for the Unruh engine.Comment: 31 pages, 11 figure
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