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We live in an exciting time for cosmology. After decades of struggling to obtain data about the properties of our universe on the largest scales and at the earliest possible times, we now find ourselves with a wealth of data pouring in from many sources. These include observations of the microwave background radiation — the relic radiation of the early universe — and surveys of astronomical objects — galaxies, quasars, supernovae, gamma-ray bursters, … — over large fractions of the sky out to large fractions of the radius of the observable universe. This flow of data is likely to only increase — new larger, deeper surveys, more detailed observations of the microwave background and its polarization, measurements of gravitational lensing, observations of gravity waves.
At the same time, precision tests of our fundamental theories of particle physics and of gravity continue to improve. The Standard Model (SM) of the strong, weak, and electromagnetic interactions of particles is a remarkable achievement; after thirty years of being tested, its predictions still agree with all known experimental data within the limits of experimental and theoretical accuracy. In all that time, the only twist that data has forced us to add to the theory is neutrino masses, and those slip into the theory so easily that it is almost unfair to call them non-Standard Model.
At the same time, precision tests of our fundamental theories of particle physics and of gravity continue to improve. The Standard Model (SM) of the strong, weak, and electromagnetic interactions of particles is a remarkable achievement; after thirty years of being tested, its predictions still agree with all known experimental data within the limits of experimental and theoretical accuracy. In all that time, the only twist that data has forced us to add to the theory is neutrino masses, and those slip into the theory so easily that it is almost unfair to call them non-Standard Model.
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Quinn Taylor,Glenn D. Starkman, Michael Hinczewski, Deyan P. Mihaylov,Joseph Silk, Jose de Freitas Pacheco
arxiv(2024)
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arxiv(2024)
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 3 (2024): 2274-2288
Deyan P. Mihaylov,Yashar Akrami,Craig J. Copi,Andrew H. Jaffe,Arthur Kosowsky,Pip Petersen,Glenn D. Starkman,Andrius Tamosiunas,Johannes R. Eskilt,Özenç Güngör, Samanta Saha,Quinn Taylor
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICSno. 2 (2023)
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Stefano Anselmi, M. F. Carney,John T. Giblin,Saurabh Kumar,James B. Mertens, M.A. O'Dwyer,Glenn D. Starkman,Chi Tian
Journal of Cosmology and Astroparticle Physicsno. 02 (2023): 049-049
Johannes R. Eskilt,Yashar Akrami,Stefano Anselmi,Craig J. Copi,Andrew H. Jaffe,Arthur Kosowsky, Deyan P. Mihaylov,Glenn D. Starkman,Andrius Tamosiunas,James B. Mertens,Pip Petersen, Samanta Saha,
arxiv(2023)
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