6,391 research outputs found

    Dust of Dark Energy

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    We introduce a novel class of field theories where energy always flows along timelike geodesics, mimicking in that respect dust, yet which possess non-zero pressure. This theory comprises two scalar fields, one of which is a Lagrange multiplier enforcing a constraint between the other's field value and derivative. We show that this system possesses no wave-like modes but retains a single dynamical degree of freedom. Thus, the sound speed is always identically zero on all backgrounds. In particular, cosmological perturbations reproduce the standard behaviour for hydrodynamics with vanishing sound speed. Using all these properties we propose a model unifying Dark Matter and Dark Energy in a single degree of freedom. In a certain limit this model exactly reproduces the evolution history of Lambda-CDM, while deviations away from the standard expansion history produce a potentially measurable difference in the evolution of structure.Comment: 13 pages, 3 figures. Added references, corrected language

    Perbandingan Pemberian Antibiotik Profilaksis Ceftriaxon Dan Non-ceftriaxon Terhadap Kejadian Surgical Site Infection Pasca Kolesistektomi

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    Latar belakang : Surgical Site Infection (SSI) merupakan salah satu komplikasi pascaoperasi yang harus dihindari. Penggunaan antibiotik profilaksis diharapkan dapat mengurangi kejadian SSI. Pemilihan jenis antibiotik profilaksis yang tepat dibutuhkan agar penggunaan antibiotik menjadi rasional dan efektif.Tujuan : Membandingkan pemberian antibiotik profilaksis ceftriaxone dan non ceftriaxone terhadap kejadian SSI pada pasien kolesistolitiasis yang dilakukan laparoskopi dan laparotomi kolesistektomi.Metode : Penelitian ini merupakan penelitian observasional dengan metode penelitian cross sectional, dilaksanakan di bagian rekam medik RSUP Dr. Kariadi Semarang. Pasien dibagi menjadi kelompok yang diberikan antibiotik ceftriaxone dan non ceftriaxone baik yang dilakukan laparoskopi kolesistektomi atau laparotomi kolesistektomi. Data tersebut dianalisis dengan uji Fisher dan perhitungan risiko dengan Prevalnce Ratio menggunakan tabel 2x2.Hasil : Diantara variabel yang diteliti hanya variabel jenis kelamin yang bermakna dengan nilai p = 0,023. Sedangkan untuk perbedaan jenis pemberian antibiotik profilaksis (p = 0,636) dan jenis tindakan operasi (p = 0,066) tidak bermakna. Uji regresi logistik untuk variabel jenis kelamin dan umur tidak bisa dilakukan. Jenis operasi laparotomi kolesistektomi memiliki risiko 4,583 lebih besar untuk terjadinya SSI (Interval Kepercayaan 95% = 1,050 - 20,003)Kesimpulan : Tidak ada perbedaan yang bermakna antara pemberian antibiotik profilaksis ceftriaxone dan non ceftriaxone pada pasien kolesistolitiasis yang dilakukan laparoskopi atau laparotomi kolesistektomi terhadap kejadian SSI

    Probabilities in the inflationary multiverse

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    Inflationary cosmology leads to the picture of a "multiverse," involving an infinite number of (spatially infinite) post-inflationary thermalized regions, called pocket universes. In the context of theories with many vacua, such as the landscape of string theory, the effective constants of Nature are randomized by quantum processes during inflation. We discuss an analytic estimate for the volume distribution of the constants within each pocket universe. This is based on the conjecture that the field distribution is approximately ergodic in the diffusion regime, when the dynamics of the fields is dominated by quantum fluctuations (rather than by the classical drift). We then propose a method for determining the relative abundances of different types of pocket universes. Both ingredients are combined into an expression for the distribution of the constants in pocket universes of all types.Comment: 18 pages, RevTeX 4, 2 figures. Discussion of the full probability in Sec.VI is sharpened; the conclusions are strengthened. Note added explaining the relation to recent work by Easther, Lim and Martin. Some references adde

    Decomposition of homogeneous polynomials with low rank

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    Let FF be a homogeneous polynomial of degree dd in m+1m+1 variables defined over an algebraically closed field of characteristic zero and suppose that FF belongs to the ss-th secant varieties of the standard Veronese variety Xm,d⊂P(m+dd)−1X_{m,d}\subset \mathbb{P}^{{m+d\choose d}-1} but that its minimal decomposition as a sum of dd-th powers of linear forms M1,...,MrM_1, ..., M_r is F=M1d+...+MrdF=M_1^d+... + M_r^d with r>sr>s. We show that if s+r≀2d+1s+r\leq 2d+1 then such a decomposition of FF can be split in two parts: one of them is made by linear forms that can be written using only two variables, the other part is uniquely determined once one has fixed the first part. We also obtain a uniqueness theorem for the minimal decomposition of FF if the rank is at most dd and a mild condition is satisfied.Comment: final version. Math. Z. (to appear

    Influence of the Fermi Surface Morphology on the Magnetic Field-Driven Vortex Lattice Structure Transitions in YBa2_{2}Cu3_{3}O7−ή:ή=_{7-\delta}:\delta=0, 0.15

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    We report small-angle neutron scattering measurements of the vortex lattice (VL) structure in single crystals of the lightly underdoped cuprate superconductor YBa2Cu3O6.85. At 2 K, and for fields of up to 16 T applied parallel to the crystal c-axis, we observe a sequence of field-driven and first-order transitions between different VL structures. By rotating the field away from the c-axis, we observe each structure transition to shift to either higher or lower field dependent on whether the field is rotated towards the [100] or [010] direction. We use this latter observation to argue that the Fermi surface morphology must play a key role in the mechanisms that drive the VL structure transitions. Furthermore, we show this interpretation is compatible with analogous results obtained previously on lightly overdoped YBa2Cu3O7. In that material, it has long-been suggested that the high field VL structure transition is driven by the nodal gap anisotropy. In contrast, the results and discussion presented here bring into question the role, if any, of a nodal gap anisotropy on the VL structure transitions in both YBa2Cu3O6.85 and YBa2Cu3O7

    Imperfect Dark Energy from Kinetic Gravity Braiding

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    We introduce a large class of scalar-tensor models with interactions containing the second derivatives of the scalar field but not leading to additional degrees of freedom. These models exhibit peculiar features, such as an essential mixing of scalar and tensor kinetic terms, which we have named kinetic braiding. This braiding causes the scalar stress tensor to deviate from the perfect-fluid form. Cosmology in these models possesses a rich phenomenology, even in the limit where the scalar is an exact Goldstone boson. Generically, there are attractor solutions where the scalar monitors the behaviour of external matter. Because of the kinetic braiding, the position of the attractor depends both on the form of the Lagrangian and on the external energy density. The late-time asymptotic of these cosmologies is a de Sitter state. The scalar can exhibit phantom behaviour and is able to cross the phantom divide with neither ghosts nor gradient instabilities. These features provide a new class of models for Dark Energy. As an example, we study in detail a simple one-parameter model. The possible observational signatures of this model include a sizeable Early Dark Energy and a specific equation of state evolving into the final de-Sitter state from a healthy phantom regime.Comment: 41 pages, 7 figures. References and some clarifying language added. This version was accepted for publication in JCA
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