نتایج جستجو برای: Space-like hypersurface

تعداد نتایج: 1114039  

Journal: :bulletin of the iranian mathematical society 2011
s. shu a. yi han

Journal: :Universe 2023

We introduce the generalized helical hypersurface having a space-like axis in five-dimensional Minkowski space. compute first and second fundamental form matrices, Gauss map, shape operator matrix of hypersurface. Additionally, we curvatures by using Cayley–Hamilton theorem. Moreover, give some relations for mean Gauss–Kronecker Finally, obtain Laplace–Beltrami

2005
Hyang Sook Kim Young-Mi Kim

In this paper, we find an upper bound of the squared norm of the second fundamental tensor of a complete space-like hypersurface in a Lorentz space form M 1 (c) satisfying some curvature conditions . Then it gives naturally an extension of some theorems of Cheng and Nakagawa ([3]), Ishihara ([7]), Li ([8]) and Nishikawa ([9]). Mathematics Subject Classification: 53C50, 53C25, 53C42.

Journal: :bulletin of the iranian mathematical society 0
s. k. hui department of mathematics, sidho kanho birsha university, purulia-723104, west bengal, india.newline department of mathematics, bankura university, bankura-722155, west bengal, india. y. matsuyama department of mathematics, chuo university, faculty of science and engineering, 1-13-27 kasuga, bunkyo-ku, tokyo 112-8551, japan.

pseudo ricci symmetric real hypersurfaces of a complex projective space are classified and it is proved that there are no pseudo ricci symmetric real hypersurfaces of the complex projective space cpn for which the vector field ξ from the almost contact metric structure (φ, ξ, η, g) is a principal curvature vector field.

1999
W Greiner

Freeze-out of particles in relativistic hydrodynamics is considered across a 3-dimensional space-time hypersurface. The conservation laws for time-like parts of the freeze-out hypersurface require different values of temperature, baryonic chemical potential and flow velocity in the fluid and in the final particle spectra. We analyze this freeze-out discontinuity and its connection to the shock-...

1996
Edward Malec

We investigate the Cauchy problem for the Einstein scalar field equations in asymptotically flat spherically symmetric spacetimes, in the standard 1+3 formulation. We prove the local existence and uniqueness of solutions for initial data given on a space-like hypersurface in the Sobolev H1∩H1,4 space. Solutions exist globally if a central (integral) singularity does not form and/or outside an o...

Let M^2n be a hoph hypersurfaces with parallel ricci operator and tangent to structure vector field in Sasakian space form. First, we show that structures and properties of hypersurfaces and hoph hypersurfaces in Sasakian space form. Then we study the structure of hypersurfaces and hoph hypersurfaces with a parallel ricci tensor structure and show that there are two cases. In the first case, th...

Let $(M^{2n},g)$ be a real hypersurface with recurrent shapeoperator and tangent to the structure vector field $xi$ of the Sasakian space form$widetilde{M}(c)$. We show that if the shape operator $A$ of $M$ isrecurrent then it is parallel. Moreover, we show that $M$is locally a product of two constant $phi-$sectional curvaturespaces.

Journal: :bulletin of the iranian mathematical society 2013
f. pashaie s.m.b. kashani

we study connected orientable spacelike hypersurfaces $x:m^{n}rightarrowm_q^{n+1}(c)$, isometrically immersed into the riemannian or lorentzian space form of curvature $c=-1,0,1$, and index $q=0,1$, satisfying the condition $~l_kx=ax+b$,~ where $l_k$ is the $textit{linearized operator}$ of the $(k+1)$-th mean curvature $h_{k+1}$ of the hypersurface for a fixed integer $0leq k

1999
Kyrill A. Bugaev

The particle emission in relativistic hydrodynamic model is formulated assuming a sharp 3-dimensional space-time freeze-out hypersurface. The boundary conditions correspond to the energy-momentum and charge conservation between fluid and the gas of free particles . The emission and possible feedback of particles are included into the self-consistent hydrodynamic scheme. For the time-like parts ...

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