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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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The International School for Advanced Studies (SISSA) was founded in 1978 and was the first institution in Italy to promote post-graduate courses leading to a Doctor Philosophiae (or PhD) degree. A centre of excellence among Italian and international universities, the school has around 65 teachers, 100 post docs and 245 PhD students, and is located in Trieste, in a campus of more than 10.
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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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[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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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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[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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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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Lamoraal Ulbo de Sitter became well-known as a structural geologist and died in Nistelrode in 1980. Aernout de Sitter served as director of the Bosscha Observatory in Lembang, Dutch East Indies. After the Japanese invasion of the Dutch East Indies he was arrested and put into a detention camp where he died on 5 September 1944.
