3,851 research outputs found

    Above the Law: The Prosecutor\u27s Duty to Seek Justice and the Performance of Substantial Assistance Agreements

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    We study the gravitational-wave (GW) signatures of clouds of ultralight bosons around black holes (BHs) in binary inspirals. These clouds, which are formed via superradiance instabilities for rapidly rotating BHs, produce distinct effects in the population of BH masses and spins, and, for real fields, a continuous monochromatic GW signal. We show that the presence of a binary companion greatly enriches the dynamical evolution of the system, most remarkably through the existence of resonant transitions between the growing and decaying modes of the cloud (analogous to Rabi oscillations in atomic physics). These resonances have rich phenomenological implications for current and future GW detectors. Notably, the amplitude of the GW signal from the clouds may be reduced, and in many cases terminated, much before the binary merger. The presence of a boson cloud can also be revealed in the GW signal from the binary through the imprint of finite-size effects, such as spin-induced multipole moments and tidal Love numbers. The time dependence of the cloud's energy density during the resonance leads to a sharp feature, or at least attenuation, in the contribution from the finite-size terms to the waveforms. The observation of these effects would constrain the properties of putative ultralight bosons through precision GW data, offering new probes of physics beyond the Standard Model

    Randomized benchmarking of atomic qubits in an optical lattice

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    We perform randomized benchmarking on neutral atomic quantum bits (qubits) confined in an optical lattice. Single qubit gates are implemented using microwaves, resulting in a measured error per randomized computational gate of 1.4(1) x 10^-4 that is dominated by the system T2 relaxation time. The results demonstrate the robustness of the system, and its viability for more advanced quantum information protocols.Comment: 11 pages, 4 figure

    Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order

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    Using effective field theory techniques we calculate the source multipole moments needed to obtain the spin contributions to the power radiated in gravitational waves from inspiralling compact binaries to third Post-Newtonian order (3PN). The multipoles depend linearly and quadratically on the spins and include both spin(1)spin(2) and spin(1)spin(1) components. The results in this paper provide the last missing ingredient required to determine the phase evolution to 3PN including all spin effects which we will report in a separate paper.Comment: 35 pages, 7 figures. Published versio

    Produtividade e valor nutritivo das frações forrageiras da erva-sal (Atriplex nummularia) irrigada com quatro diferentes volumes de efluentes da criação de tilápia em água salobra.

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    Avaliou-se a produtividade e o valor nutritivo da erva sal cultivada sob irrigação de quatro volumes de efluentes oriundos de viveiros de criação de tilápia (Oreochromis sp.), cuja salinidade média durante o cultivo foi de 8,29 dS m-l. O delíneamento experimental foi de blocos ao acaso com quatrO tratamentos e três repetições. Os tratamentos de 75, 150, 225 e 300 litros de efluente por planta foram aplicados semanalmente. Os diferentes volumes de água influenciaram a produtividade de matéria seca, mas não influenciaram a composição químico-bromatológica e digestibilidade in vitro da matéria seca em qualquer dos componentes da planta. Os teores de minerais (MM) mostraram-se elevados nas folhas, requerendo assim, cuidados com dietas contendo alta proporção de folhas de erva sal, a ponto de não permitir que teores elevados de sais sejam comprometedores do consumo animal. O teor de proteína bruta e digestibilidade ín vítro da matéria seca médio dos tratamentos para as folhas foi de 15,1 e 67,9%, respectivamente. Ramos e Caules apresentaram elevados teores de FDN e FDA e baixos valores de DIVMS. Independente do nível de água aplicado, a erva sal mostrou características forrageiras desejável, que podem ainda ser melhoradas com práticas de manejo voltadas para tal fim

    Captação de Fucsina ácida em gemas de macieira em diferentes estádios de dormência.

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    No presente trabalho, avaliou-se a fucsina como indicadora do estádio de dormência, objetivando otimizar um método para aplicação e avaliação do corante nos tecidos, paralelamente com a obtenção de resultados de brotação forçada.Resumo

    A multi-photon magneto-optical trap

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    We demonstrate a Magneto-Optical Trap (MOT) configuration which employs optical forces due to light scattering between electronically excited states of the atom. With the standard MOT laser beams propagating along the {\it x}- and {\it y}- directions, the laser beams along the {\it z}-direction are at a different wavelength that couples two sets of {\it excited} states. We demonstrate efficient cooling and trapping of cesium atoms in a vapor cell and sub-Doppler cooling on both the red and blue sides of the two-photon resonance. The technique demonstrated in this work may have applications in background-free detection of trapped atoms, and in assisting laser-cooling and trapping of certain atomic species that require cooling lasers at inconvenient wavelengths.Comment: 10 pages, 5 figure

    Strongly inhibited transport of a 1D Bose gas in a lattice

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    We report the observation of strongly damped dipole oscillations of a quantum degenerate 1D atomic Bose gas in a combined harmonic and optical lattice potential. Damping is significant for very shallow axial lattices (0.25 photon recoil energies), and increases dramatically with increasing lattice depth, such that the gas becomes nearly immobile for times an order of magnitude longer than the single-particle tunneling time. Surprisingly, we see no broadening of the atomic quasimomentum distribution after damped motion. Recent theoretical work suggests that quantum fluctuations can strongly damp dipole oscillations of 1D atomic Bose gas, providing a possible explanation for our observations.Comment: 5 pages, 4 figure
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