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book (4)


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English (4)


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2022 (4)

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Book
Exact Solutions in Classical Field Theory: Solitons, Black Holes and Boson Stars
Authors: ---
Year: 2022 Publisher: Basel MDPI - Multidisciplinary Digital Publishing Institute

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Abstract

Special Issue in honour of Prof. Yves Brihaye, on the occasion of his 65th birthday. The issue is mainly dedicated to the study of compact objects and solutions to Einstein-Yang-Mills equations and extensions thereof, topics to which Prof. Y. Brihaye contributed very significantly.


Book
Exact Solutions in Classical Field Theory: Solitons, Black Holes and Boson Stars
Authors: ---
Year: 2022 Publisher: Basel MDPI - Multidisciplinary Digital Publishing Institute

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Abstract

Special Issue in honour of Prof. Yves Brihaye, on the occasion of his 65th birthday. The issue is mainly dedicated to the study of compact objects and solutions to Einstein-Yang-Mills equations and extensions thereof, topics to which Prof. Y. Brihaye contributed very significantly.


Book
Exact Solutions in Classical Field Theory: Solitons, Black Holes and Boson Stars
Authors: ---
Year: 2022 Publisher: Basel MDPI - Multidisciplinary Digital Publishing Institute

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Bookmark

Abstract

Special Issue in honour of Prof. Yves Brihaye, on the occasion of his 65th birthday. The issue is mainly dedicated to the study of compact objects and solutions to Einstein-Yang-Mills equations and extensions thereof, topics to which Prof. Y. Brihaye contributed very significantly.


Book
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars
Authors: ---
ISBN: 3036554009 3036553991 Year: 2022 Publisher: MDPI - Multidisciplinary Digital Publishing Institute

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Abstract

Following new developments in the measurement of gravitational waves from neutron–star mergers and the modification or construction of particle colliders to reach larger densities, we are entering a new era, during which we can begin to understand dense and hot matter for the first time. This, together with future supernova explosion data, will provide us with the opportunity to have truly multimessenger data on hot and dense matter, which is, to some extent, similar to the matter present in the core of proto-neutron stars. This Special Issue focuses on the theory necessary to understand present and future data. It includes state-of-the-art theoretical models that describe dense and hot matter and dynamical stellar simulations that make use of them, with the ultimate goal of determining which degrees of freedom are relevant under these conditions and how they affect the matter equation of state and stellar evolution.

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