885 research outputs found

    String is a double slit

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    We perform imaging of a fundamental string from string scattering amplitudes, and show that its image is a double slit

    ビナフトール - チタン ルイスサン オ モチイタ アルファ ベータ - フホウワ アルデヒド ノ ショクバイテキ フセイ 1 3 - ソウキョクシ フカ カンカ ハンノウ ノ カイハツ

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    京都大学0048新制・課程博士博士(理学)甲第12135号理博第3029号新制||理||1451(附属図書館)UT51-2006-J129京都大学大学院理学研究科化学専攻(主査)教授 丸岡 啓二, 教授 林 民生, 教授 大須賀 篤弘学位規則第4条第1項該当Doctor of ScienceKyoto UniversityDFA

    Simulation of an interlocking hydraulic direct-drive system for a biped walking robot

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    Biped robots with serial links driven by an electric motor experience problems because the motor and transmission are installed in each joint, causing the legs to become very heavy. Previous solutions involved robots using servo valves, a type of highly responsive proportional valve. However, high supply pressure is necessary to realize high responsiveness and the resulting energy losses are large. To address this problem, we proposed a hydraulic direct-drive system in which the pump controls the cylinder meter-in flow, while a proportional valve controls the meter-out flow. Furthermore, our hydraulic interlocking drive system connects two hydraulic direct-drive systems for biped humanoid robots and concentrates the pump output on one side cylinder. The meter-in flow rate of the other side cylinder is controlled by the meter-out flow rate of the cylinder on which the pump is concentrated. A comparison of the walking simulation performance with that of the conventional independent system shows that our proposed system reduces the motor output power by 24.3%. These results prove the feasibility of constructing a two-legged robot without having to incorporate highly responsive servo valves

    Topology conserving gauge action and the overlap-Dirac operator

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    We apply the topology conserving gauge action proposed by Luescher to the four-dimensional lattice QCD simulation in the quenched approximation. With this gauge action the topological charge is stabilized along the hybrid Monte Carlo updates compared to the standard Wilson gauge action. The quark potential and renormalized coupling constant are in good agreement with the results obtained with the Wilson gauge action. We also investigate the low-lying eigenvalue distribution of the hermitian Wilson-Dirac operator, which is relevant for the construction of the overlap-Dirac operator.Comment: 27pages, 11figures, accepted versio

    The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at z2z\sim2

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    We present average stellar population properties and dark matter halo masses of z2z \sim 2 \lya emitters (LAEs) from SED fitting and clustering analysis, respectively, using \simeq 12501250 objects (NB38725.5NB387\le25.5) in four separate fields of 1\simeq 1 deg2^2 in total. With an average stellar mass of 10.2±1.8×108 M10.2\, \pm\, 1.8\times 10^8\ {\mathrm M_\odot} and star formation rate of 3.4±0.4 M yr13.4\, \pm\, 0.4\ {\mathrm M_\odot}\ {\rm yr^{-1}}, the LAEs lie on an extrapolation of the star-formation main sequence (MS) to low stellar mass. Their effective dark matter halo mass is estimated to be $4.0_{-2.9}^{+5.1} \times 10^{10}\ {\mathrm M_\odot}withaneffectivebiasof with an effective bias of 1.22^{+0.16}_{-0.18}whichislowerthanthatof which is lower than that of z \sim 2LAEs( LAEs (1.8\, \pm\, 0.3),obtainedbyapreviousstudybasedonathreetimessmallersurveyarea,withaprobabilityof), obtained by a previous study based on a three times smaller survey area, with a probability of 96\%. However, the difference in the bias values can be explained if cosmic variance is taken into account. If such a low halo mass implies a low HI gas mass, this result appears to be consistent with the observations of a high \lya escape fraction. With the low halo masses and ongoing star formation, our LAEs have a relatively high stellar-to-halo mass ratio (SHMR) and a high efficiency of converting baryons into stars. The extended Press-Schechter formalism predicts that at z=0ourLAEsaretypicallyembeddedinhaloswithmassessimilartothatoftheLargeMagellanicCloud(LMC);theywillalsohavesimilarSHMRstotheLMC,iftheirSFRsarelargelysuppressedafter our LAEs are typically embedded in halos with masses similar to that of the Large Magellanic Cloud (LMC); they will also have similar SHMRs to the LMC, if their SFRs are largely suppressed after z \sim 2$ as some previous studies have reported for the LMC itself.Comment: 34 pages, 15 figures, 6 tables. Accepted for publication in PAS
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