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      Quantum phase estimation using path-symmetric entangled states

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          Abstract

          We study the sensitivity of phase estimation using a generic class of path-symmetric entangled states \(|\varphi\rangle|0\rangle+|0\rangle|\varphi\rangle\), where an arbitrary state \(|\varphi\rangle\) occupies one of two modes in quantum superposition. This class of states includes the previously considered states, i.e. \(NOON\) states and entangled coherent states, as special cases. With its generalization, we identify the practical limit of phase estimation under energy constraint that is characterized by the photon statistics of the component state \(|\varphi\rangle\). We first show that quantum Cramer-Rao bound (QCRB) can be lowered with super-Poissonianity of the state \(|\varphi\rangle\). By introducing a component state of the form \(|\varphi\rangle=\sqrt{q}|1\rangle+\sqrt{1-q}|N\rangle\), we particularly show that an arbitrarily small QCRB can be achieved even with a finite energy in an ideal situation. For practical measurement schemes, we consider a parity measurement and a full photon-counting method to obtain phase-sensitivity. Without photon loss, the latter scheme employing any path-symmetric states \(|\varphi\rangle|0\rangle+|0\rangle|\varphi\rangle\) achieves the QCRB over the entire range \([0,2\pi]\) of unknown phase shift \(\phi\) whereas the former does so in a certain confined range of \(\phi\). We find that the case of \(|\varphi\rangle=\sqrt{q}|1\rangle+\sqrt{1-q}|N\rangle\) provides the most robust resource against loss among the considered entangled states over the whole range of input energy. Finally we also propose experimental schemes to generate these path-symmetric entangled states.

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          Observation of Gravitational Waves from a Binary Black Hole Merger

          On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of \(1.0 \times 10^{-21}\). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater than 5.1 {\sigma}. The source lies at a luminosity distance of \(410^{+160}_{-180}\) Mpc corresponding to a redshift \(z = 0.09^{+0.03}_{-0.04}\). In the source frame, the initial black hole masses are \(36^{+5}_{-4} M_\odot\) and \(29^{+4}_{-4} M_\odot\), and the final black hole mass is \(62^{+4}_{-4} M_\odot\), with \(3.0^{+0.5}_{-0.5} M_\odot c^2\) radiated in gravitational waves. All uncertainties define 90% credible intervals.These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.
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            Advances in Quantum Metrology

            In classical estimation theory, the central limit theorem implies that the statistical error in a measurement outcome can be reduced by an amount proportional to n^(-1/2) by repeating the measures n times and then averaging. Using quantum effects, such as entanglement, it is often possible to do better, decreasing the error by an amount proportional to 1/n. Quantum metrology is the study of those quantum techniques that allow one to gain advantages over purely classical approaches. In this review, we analyze some of the most promising recent developments in this research field. Specifically, we deal with the developments of the theory and point out some of the new experiments. Then we look at one of the main new trends of the field, the analysis of how the theory must take into account the presence of noise and experimental imperfections.
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              Deterministically encoding quantum information using 100-photon Schrödinger cat states.

              In contrast to a single quantum bit, an oscillator can store multiple excitations and coherences provided one has the ability to generate and manipulate complex multiphoton states. We demonstrate multiphoton control by using a superconducting transmon qubit coupled to a waveguide cavity resonator with a highly ideal off-resonant coupling. This dispersive interaction is much greater than decoherence rates and higher-order nonlinearities to allow simultaneous manipulation of hundreds of photons. With a tool set of conditional qubit-photon logic, we mapped an arbitrary qubit state to a superposition of coherent states, known as a "cat state." We created cat states as large as 111 photons and extended this protocol to create superpositions of up to four coherent states. This control creates a powerful interface between discrete and continuous variable quantum computation and could enable applications in metrology and quantum information processing.
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                Author and article information

                Journal
                2015-05-22
                2015-10-28
                Article
                10.1038/srep30306
                1505.06000
                a46437de-7b57-4328-83c7-8002a7d2c215

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                7 pages, 8 figures, title changed, references and new material added
                quant-ph

                Quantum physics & Field theory
                Quantum physics & Field theory

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