نتایج جستجو برای: newton cotes

تعداد نتایج: 20096  

Journal: :Thermal Science 2021

One 3-D transient temperature field model for a thin uniform plate caused by moving laser heat source is described in present study. The with power density Gaussian-distribution form considered when finite-thin heated. By using the separate variable method and Newton-Cotes method, semi-analytical solution of conduction equation finite obtained. Numerical results show that effect distribution, s...

2006
M. Perri D. Guetta L. A. Antonelli A. Cucchiara V. Mangano J. Reeves L. Angelini A. P. Beardmore P. Boyd D. N. Burrows S. Campana M. Capalbi G. Chincarini G. Cusumano P. Giommi J. E. Hill S. T. Holland V. La Parola T. Mineo A. Moretti J. A. Nousek J. P. Osborne C. Pagani P. Romano P. W. A. Roming R. L. C. Starling G. Tagliaferri E. Troja L. Vetere N. Gehrels

Aims. We observed the high redshift (z = 3.969) GRB 050730 with Swift and XMM-Newton to study its prompt and afterglow emission. Methods. We carried out a detailed spectral and temporal analysis of Swift and XMM-Newton observations. Results. The X–ray afterglow of GRB 050730 was found to decline with time with superimposed intense flaring activity that extended over more than two orders of magn...

2012
EVA VIEHMANN

We generalize purity of the Newton stratification to purity for a single break point of the Newton point in the context of local G-shtukas respectively of elements of the loop group of a reductive group. As an application we prove that elements of the loop group bounded by a given dominant coweight satisfy a generalization of Grothendieck’s conjecture on deformations of p-divisible groups with ...

2001
G. Ramm

Suppose that the inverse scattering problem is understood as follows: given fixed-energy phase shifts, corresponding to an unknown potential q = q(r) from a certain class, for example, q ∈ L 1,1 , recover this potential. Then it is proved that the Newton-Sabatier (NS) procedure does not solve the above problem. It is not a valid inversion method, in the following sense: 1) it is not possible to...

2001
S. Mereghetti

We report on an observation of the Anomalous X– ray Pulsar 1E 1048.1–5937 performed with the XMM-Newton satellite. The phase averaged spectrum of 1E 1048.1–5937 is well described by the sum of a power law with photon index ∼2.9 and a blackbody with temperature ∼0.6 keV, without evidence for significant absorption or emission lines. The above spectral parameters do not vary during the phases cor...

2012
Simon Saunders

It is widely accepted that the notion of inertial frame is central to Newtonian mechanics, and that the correct space-time structure underlying Newton’s methods in Principia is neo-Newtonian or Galilean space-time. I argue to the contrary that inertial frames are not needed in Newton’s theory of motion, and that the right space-time structure for Newton’s Principia requires the notion of parall...

2004
OLGA HOLTZ

Newton’s inequalities cn ≥ cn−1cn+1 are shown to hold for the normalized coefficients cn of the characteristic polynomial of any Mor inverse M-matrix. They are derived by establishing first an auxiliary set of inequalities also valid for both of these classes. They are also used to derive some new necessary conditions on the eigenvalues of nonnegative matrices.

2017
C. Duval G. W. Gibbons P. A. Horváthy

Definitions of non-relativistic conformal transformations are considered both in the Newton-Cartan and in the Kaluza-Klein-type Eisenhart/Bargmann geometrical frameworks. The symmetry groups that come into play are exemplified by the cosmological, and also the Newton-Hooke solutions of Newton’s gravitational field equations. It is shown, in particular, that the maximal symmetry group of the sta...

Journal: :Journal of Computational and Applied Mathematics 1996

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