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SITTER, WILLEM DE. ( b. Sneek, Netherlands, 6 May 1872; d. Leiden, Netherlands, 20 November 1934) astronomy. De Sitter was the son of L. U. De sitter, a judge, who became president of the court at Arnhem, and T. W. S. Bertling. After preparatory education at Arnhem he entered the University of Groningen, where he studied mathematics and physics.
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Also the di erent coordinate systems for de Sitter space-time are considered. The symmetry group of the de Sitter space-time is obtained in chapter three and it is ex-plained how these transformations can preserve a minimum length. Asymptotically at [8,13,19{22] and de Sitter space-times [9,10,23{29] are considered in chapter four. 5
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A bstract. In this paper, we derive a soft photon theorem and a soft gluon theorem in the de Sitter spacetime from the Ward identity of the near cosmological horizon large gauge transformation. Taking the flat limit of the de Sitter spacetime, the soft theorems naturally recover the corresponding flat spacetime soft theorems.
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Our method is based on the Mellin-Barnes representation of correlation functions, which allows us to regulate loop divergences by adjusting the masses of the fields, or by gently deforming the underlying de Sitter spacetime. The resulting expressions have a similar structure as a standard answer from dimensional regularization in flat space QFT.
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[en] It is shown that, for a de Sitter Universe, the Hartle-Hawking (HH) wave function can be obtained in a simple way starting from the Friedmann-Lemaitre-Robertson-Walker (FLRW) line element of cosmological equations. An oscillator having imaginary time is indeed derived starting from the Hamiltonian obtaining the HH condition. This proposes again some crucial matter on the meaning.
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De Sitter Bloemen Uitvaart Bloemen voor uitvaart
of de Sitter space time as well as in primordial cosmology set up. We have constructed the maximally entangled state which suffice the purpose. But this could not be possible just having usual interaction in the scalar field theory embedded in the global patch of the de Sitter space. The Bell's CHSH inequality violating pair is created
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to (anti-)de Sitter space, and their corresponding supersymmetric generalisations. In particular, we will compute the projection operators in three-dimensional N= 0 and N= 1 AdS (super)space and four-dimensional N-extended AdS superspace for N= 1 and N= 2. We will also initiate the construction of the superspin projectors in 3d N= (1,1) AdS.
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[en] The Hawking-Page (HP) phase transitions of the anti-de Sitter black holes in the extended phase space are studied in a novel four-dimensional Einstein-Gauss-Bonnet (4EGB) gravity, which is proposed by rescaling the Gauss-Bonnet (GB) coupling constant α → α ∕ (d − 4) in d dimensions and redefining the four-dimensional gravity in the limit d → 4.
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