14,562 research outputs found

    Localized Activation of Bending in Proximal, Medial and Distal Regions of Sea-Urchin Sperm Flagella

    Get PDF
    Spermatozoa from the sea urchin, Colobocentrotus atratus, were partially demembranated by extraction with solutions containing Triton X-100 at a concentration which was insufficient to solubilize the membranes completely. The resulting suspension was a mixture containing some spermatozoa in which a proximal, medial, or distal portion of the flagellum was membrane-covered, while the remaining portion was naked axoneme. In reactivating solutions containing 12 µM ATP, only the naked portions of the flagellum became motile. In reactivating solutions containing 0.8 mM ADP, the membrane-covered regions became motile and beat at 6-10 beats/s, while the naked regions remained immobile, or beat very slowly at about 0.3 beat/s. Activation of membrane-covered regions in ADP solutions probably results from the membrane restricting the diffusion of ATP which is formed from ADP by the axonemal adenylate kinase. The results indicate that any region of the flagellum has the capacity for autonomous beating, and that special properties of the basal end of the flagellum are not required for bend initiation. However, the beating of different regions of the flagellum is not completely independent, for in a fair number of spermatozoa the beating of the distal, membrane-covered region in 0.8 mM ADP was intermittent, and was turned on and off in phase with the much slower bending cycle in the proximal region of naked axoneme

    Moduli, Scalar Charges, and the First Law of Black Hole Thermodynamics

    Get PDF
    We show that under variation of moduli fields ϕ\phi the first law of black hole thermodynamics becomes dM=κdA8π+ΩdJ+ψdq+χdpΣdϕdM = {\kappa dA\over 8\pi} + \Omega dJ + \psi dq + \chi dp - \Sigma d\phi, where Σ\Sigma are the scalar charges. We also show that the ADM mass is extremized at fixed AA, JJ, (p,q)(p,q) when the moduli fields take the fixed value ϕfix(p,q)\phi_{\rm fix}(p,q) which depend only on electric and magnetic charges. It follows that the least mass of any black hole with fixed conserved electric and magnetic charges is given by the mass of the double-extreme black hole with these charges. Our work allows us to interpret the previously established result that for all extreme black holes the moduli fields at the horizon take a value ϕ=ϕfix(p,q)\phi= \phi_{\rm fix}(p,q) depending only on the electric and magnetic conserved charges: ϕfix(p,q) \phi_{\rm fix}(p,q) is such that the scalar charges Σ(ϕfix,(p,q))=0\Sigma ( \phi_{\rm fix}, (p,q))=0.Comment: 3 pages, no figures, more detailed versio

    Critical Pebbling Numbers of Graphs

    Full text link
    We define three new pebbling parameters of a connected graph GG, the rr-, gg-, and uu-critical pebbling numbers. Together with the pebbling number, the optimal pebbling number, the number of vertices nn and the diameter dd of the graph, this yields 7 graph parameters. We determine the relationships between these parameters. We investigate properties of the rr-critical pebbling number, and distinguish between greedy graphs, thrifty graphs, and graphs for which the rr-critical pebbling number is 2d2^d.Comment: 26 page

    Black Hole Solutions of Kaluza-Klein Supergravity Theories and String Theory

    Get PDF
    We find U(1)_{E} \times U(1)_{M} non-extremal black hole solutions of 6-dimensional Kaluza-Klein supergravity theories. Extremal solutions were found by Cveti\v{c} and Youm\cite{C-Y}. Multi black hole solutions are also presented. After electro-magnetic duality transformation is performed, these multi black hole solutions are mapped into the the exact solutions found by Horowitz and Tseytlin\cite{H-T} in 5-dimensional string theory compactified into 4-dimensions. The massless fields of this theory can be embedded into the heterotic string theory compactified on a 6-torus. Rotating black hole solutions can be read off those of the heterotic string theory found by Sen\cite{Sen3}.Comment: 23 pages text(latex), a figure upon reques

    Topology, Entropy and Witten Index of Dilaton Black Holes

    Full text link
    We have found that for extreme dilaton black holes an inner boundary must be introduced in addition to the outer boundary to give an integer value to the Euler number. The resulting manifolds have (if one identifies imaginary time) topology S1×R×S2S^1 \times R \times S^2 and Euler number χ=0\chi = 0 in contrast to the non-extreme case with χ=2\chi=2. The entropy of extreme U(1)U(1) dilaton black holes is already known to be zero. We include a review of some recent ideas due to Hawking on the Reissner-Nordstr\"om case. By regarding all extreme black holes as having an inner boundary, we conclude that the entropy of {\sl all} extreme black holes, including [U(1)]2[U(1)]^2 black holes, vanishes. We discuss the relevance of this to the vanishing of quantum corrections and the idea that the functional integral for extreme holes gives a Witten Index. We have studied also the topology of ``moduli space'' of multi black holes. The quantum mechanics on black hole moduli spaces is expected to be supersymmetric despite the fact that they are not HyperK\"ahler since the corresponding geometry has torsion unlike the BPS monopole case. Finally, we describe the possibility of extreme black hole fission for states with an energy gap. The energy released, as a proportion of the initial rest mass, during the decay of an electro-magnetic black hole is 300 times greater than that released by the fission of an 235U{}^{235} U nucleus.Comment: 51 pages, 4 figures, LaTeX. Considerably extended version. New sections include discussion of the Witten index, topology of the moduli space, black hole sigma model, and black hole fission with huge energy releas

    Some Comments on Gravitational Entropy and the Inverse Mean Curvature Flow

    Get PDF
    The Geroch-Wald-Jang-Huisken-Ilmanen approach to the positive energy problem to may be extended to give a negative lower bound for the mass of asymptotically Anti-de-Sitter spacetimes containing horizons with exotic topologies having ends or infinities of the form Σg×R\Sigma_g \times {\Bbb R}, in terms of the cosmological constant. We also show how the method gives a lower bound for for the mass of time-symmetric initial data sets for black holes with vectors and scalars in terms of the mass, Z(Q,P)|Z(Q,P)| of the double extreme black hole with the same charges. I also give a lower bound for the area of an apparent horizon, and hence a lower bound for the entropy in terms of the same function Z(Q,P)|Z(Q,P)|. This shows that the so-called attractor behaviour extends beyond the static spherically symmetric case. and underscores the general importance of the function Z(Q,P)|Z(Q,P)|. There are hints that higher dimensional generalizations may involve the Yamabe conjectures.Comment: 13pp. late

    Nucleating Black Holes via Non-Orientable Instantons

    Get PDF
    We extend the analysis of black hole pair creation to include non- orientable instantons. We classify these instantons in terms of their fundamental symmetries and orientations. Many of these instantons admit the pin structure which corresponds to the fermions actually observed in nature, and so the natural objection that these manifolds do not admit spin structure may not be relevant. Furthermore, we analyse the thermodynamical properties of non-orientable black holes and find that in the non-extreme case, there are interesting modifications of the usual formulae for temperature and entropy.Comment: 27 pages LaTeX, minor typos are correcte

    Rational combinations of Betti diagrams of complete intersections

    Full text link
    We investigate decompositions of Betti diagrams over a polynomial ring within the framework of Boij-S\"oderberg theory. That is, given a Betti diagram, we determine if it is possible to decompose it into the Betti diagrams of complete intersections. To do so, we determine the extremal rays of the cone generated by the diagrams of complete intersections and provide a rudimentary algorithm for decomposition.Comment: This research was conducted at the Willamette Mathematics Consortium RE

    Entropy for dilatonic black hole

    Full text link
    The area formula for entropy is extended to the case of a dilatonic black hole. The entropy of a scalar field in the background of such a black hole is calculated semiclassically. The area and cutoff dependences are normal {\it except in the extremal case}, where the area is zero but the entropy nonzero.Comment: 13 pages (Applicability of area formula justified and a reference added

    3D printing of cement composites

    Get PDF
    The aims of this study were to investigate the feasibility of generating 3D structures directly in rapid-hardening Portland cement (RHPC) using 3D Printing (3DP) technology. 3DP is a Additive Layer Manufacturing (ALM) process that generates parts directly from CAD in a layer-wise manner. 3D structures were successfully printed using a polyvinylalcohol: RHPC ratio of 3:97 w/w, with print resolutions of better than 1mm. The test components demonstrated the manufacture of features, including off-axis holes, overhangs / undercuts etc that would not be manufacturable using simple mould tools. Samples hardened by 1 day post-build immersion in water at RT offered Modulus of Rupture (MOR) values of up to 0.8±0.1MPa, and, after 26 days immersion in water at RT, offered MOR values of 2.2±0.2MPa, similar to bassanite-based materials more typically used in 3DP (1-3 MPa). Post-curing by water immersion restructured the structure, removing the layering typical of ALM processes, and infilling porosity
    corecore