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We show that if dark energy evolves in time, its dynamical component could be dominated by a bath of dark radiation.
Relaxation of the Cosmological Constant
Tom Banks · 1984
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A Mechanism for Reducing the Value of the Cosmological Constant
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On the Anomalous Electroweak Baryon Number Nonconservation in the Early Universe
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Limits on a Lorentz and Parity Violating Modification of Electrodynamics
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Physical properties of four-dimensional superstring gravity black hole solutions
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Strong sphalerons and electroweak baryogenesis
G.F. Giudice and Mikhail E. Shaposhnikov · 1994
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Motion of Chern-Simons number at high temperatures under a chemical potential
Guy D. Moore · 1996
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Electroweak baryon number nonconservation in the early universe and in high-energy collisions
V.A. Rubakov and M.E. Shaposhnikov · 1996
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Paul J. Steinhardt and Neil Turok · 2002
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Latham A. Boyle, Robert R. Caldwell, and Marc Kamionkowski · 2002
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Lorentz invariance on trial
M. Pospelov and M. Romalis · 2004
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PTOLEMY: A Proposal for Thermal Relic Detection of Massive Neutrinos and Directional Detection of MeV Dark Matter
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Direct Detection of Spin-(In)dependent Nuclear Scattering of Sub-GeV Dark Matter Using Molecular Excitations
Rouven Essig, Jesús Pérez-Ríos, Harikrishnan Ramani, and Oren Slone · 2019
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New Extraction of the Cosmic Birefringence from the Planck 2018 Polarization Data
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Storage Ring Probes of Dark Matter and Dark Energy
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Born again universe
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Planck 2018 results. VI. Cosmological parameters
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