Detecting gravitational waves via coherence degradation induced by the Unruh effect

IF 4.8 2区 物理与天体物理 Q2 PHYSICS, PARTICLES & FIELDS
Pedro H. M. Barros, Helder A. S. Costa
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引用次数: 0

Abstract

We investigate the effects of a gravitational wave background on the coherence degradation induced by the Unruh effect of a uniformly accelerated single-qubit and quantum interferometric circuit. In both systems, we use the formalism of the evolution of the density matrix of the detector-field system, where after the interaction the field degrees of freedom are traced out to obtain the reduced density matrix of the detector. In this background, we calculate the quantum coherence and interferometric visibility in the long-wavelength regime and large interaction time. Our results indicate that the gravitational wave transfers energy to the internal states of the detector, causing, together with the Unruh effect, changes in them, amplifying the coherence degradation of the system. This amplification occurs when the polarization modes of the gravitational wave are in resonance and have modulated amplitudes. For the case of a short-wavelength, the detector does not respond to the gravitational wave because its oscillation is so fast that the detector does not have time to respond within the system timescale. Therefore, it is possible to detect the signature of gravitational waves in the coherence degradation induced by the Unruh effect within the regimes studied here.

通过昂鲁效应引起的相干退化探测引力波
我们研究了引力波背景对均匀加速的单量子比特和量子干涉电路的Unruh效应引起的相干退化的影响。在这两个系统中,我们使用了探测器-场系统密度矩阵演化的形式,在相互作用后跟踪了场的自由度,得到了探测器的密度矩阵的简化。在此背景下,我们计算了长波长和大相互作用时间下的量子相干性和干涉可见性。我们的研究结果表明,引力波将能量转移到探测器的内部状态,与Unruh效应一起引起它们的变化,放大了系统的相干性退化。这种放大发生在引力波的偏振模式共振并具有调制振幅时。对于短波长的情况,探测器对引力波没有响应,因为它的振荡太快,探测器没有时间在系统时间尺度内做出响应。因此,在本文所研究的体系中,可以检测到由Unruh效应引起的相干退化中引力波的特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
The European Physical Journal C
The European Physical Journal C 物理-物理:粒子与场物理
CiteScore
8.10
自引率
15.90%
发文量
1008
审稿时长
2-4 weeks
期刊介绍: Experimental Physics I: Accelerator Based High-Energy Physics Hadron and lepton collider physics Lepton-nucleon scattering High-energy nuclear reactions Standard model precision tests Search for new physics beyond the standard model Heavy flavour physics Neutrino properties Particle detector developments Computational methods and analysis tools Experimental Physics II: Astroparticle Physics Dark matter searches High-energy cosmic rays Double beta decay Long baseline neutrino experiments Neutrino astronomy Axions and other weakly interacting light particles Gravitational waves and observational cosmology Particle detector developments Computational methods and analysis tools Theoretical Physics I: Phenomenology of the Standard Model and Beyond Electroweak interactions Quantum chromo dynamics Heavy quark physics and quark flavour mixing Neutrino physics Phenomenology of astro- and cosmoparticle physics Meson spectroscopy and non-perturbative QCD Low-energy effective field theories Lattice field theory High temperature QCD and heavy ion physics Phenomenology of supersymmetric extensions of the SM Phenomenology of non-supersymmetric extensions of the SM Model building and alternative models of electroweak symmetry breaking Flavour physics beyond the SM Computational algorithms and tools...etc.
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