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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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About this book. This is a thorough, very readable and excellently illustrated biography of Willem de Sitter (1872-1934), one of the most influential astronomers of his time, and also a co-author and correspondent of Einstein. Authored by a physicist and skilled writer, the book gives a beautiful and accessible description of the 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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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.
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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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[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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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.