Results 11 to 20 of about 13,435 (197)
sesA: A Program for the Analytic Computation of Solvent-Excluded Surface Areas. [PDF]
sesA is an accurate and robust program for analytic computation of solvent‐excluded surface (SES) area. Its most salient feature is the computation of probe‐probe intersections by exhaustive search. Detailed comparisons with msms, the current de‐facto standard for SES area computation, show that sesA is much superior to msms.
Wang L.
europepmc +2 more sources
Neck-pinching of C P 1 -structures in the PSL 2 C -character variety. [PDF]
Abstract We characterize a certain neck‐pinching degeneration of (marked) CP1$\mathbb {C}{\rm P}^1$‐structures on a closed oriented surface S$S$ of genus at least two. In a more general setting, we take a path of CP1$\mathbb {C}{\rm P}^1$‐structures Ct(t⩾0)$C_t \nobreakspace (t \geqslant 0)$ on S$S$ that leaves every compact subset in its deformation ...
Baba S.
europepmc +2 more sources
On Cherkaev-Lurie-Milton theorem in the plane problems of linear elasticity
The paper delivers a full justification of the Cherkaev–Lurie–Milton theorem in application to the elasticity problem of in-plane loaded plates, 2D periodic elastic composites, elasticity of thin plates subjected to transverse loads as well as in-plane ...
T. Lewiński
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Gauss-Bonnet theorem in Lorentzian Sasakian space forms
In this paper, we use a Lorentzian approximation scheme to compute the sub-Lorentzian limit of curvatures for curves and Lorentzian surfaces in the Lorentzian Bianci-Cartan-Vranceanu model of 3-dimensional Lorentzian Sasakian space forms.
Haiming Liu, Jiajing Miao
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Hawking radiation via Gauss–Bonnet theorem
In this paper, we apply the topological method to the various black holes to derive their Hawking temperature. We show that the this method can easily be employed to compute the Hawking temperature of black holes having spherically symmetric topology.
A. Övgün, İ. Sakallı
openaire +3 more sources
Einstein Gauss-Bonnet theories as ordinary, Wess-Zumino conformal anomaly actions
Recently, the possibility of evading Lovelock's theorem at d=4, via a singular redefinition of the dimensionless coupling of the Gauss-Bonnet term, has been very extensively discussed in the cosmological context.
Claudio Corianò, Matteo Maria Maglio
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Hairy black-holes in shift-symmetric theories
Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem of Hui and Nicolis, assuming spherical symmetry, time-independence of the scalar field and asymptotic flatness.
Paolo Creminelli +4 more
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A consistent theory of D → 4 Einstein-Gauss-Bonnet gravity
We investigate the D→4 limit of the D-dimensional Einstein-Gauss-Bonnet gravity, where the limit is taken with α˜=(D−4)α kept fixed and α is the original Gauss-Bonnet coupling.
Katsuki Aoki +2 more
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Diving inside a hairy black hole
We investigate the interior of the Einstein-Gauss-Bonnet charged black-hole with scalar hair. We find a variety of dynamical epochs, with the particular important feature that the Cauchy horizon is not present.
Nicolás Grandi, Ignacio Salazar Landea
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Charged stars in 4D Einstein–Gauss–Bonnet gravity
An alternative gravity theory that has attracted considerable attention recently is the novel four-dimensional Einstein–Gauss–Bonnet (4EGB) gravity. This idea was proposed to bypass the Lovelock’s theorem and to permit nontrivial higher curvature effects
Ayan Banerjee +2 more
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