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Probing the dark energy: methods and strategies
Dragan Huterer, Michael S. Turner
The presence of dark energy in the Universe is inferred directly from the accelerated expansion of the Universe, and indirectly, from measurements of cosmic microwave background (C…
Big-Bang Nucleosynthesis Predictions for Precision Cosmology
Scott Burles, Kenneth M. Nollett, Michael S. Turner
The determination of the primeval deuterium abundance has opened a precision era in big-bang nucleosynthesis (BBN), making accurate predictions more important than ever before. We…
What Is The BBN Prediction for the Baryon Density and How Reliable Is It?
Scott Burles, Kenneth M. Nollett, Michael S. Turner
Together, the standard theory of big-bang nucleosynthesis (BBN) and the primeval deuterium abundance now very precisely peg the baryon density. Based upon our analysis of the deute…
Optimal Supernova Search Strategies
Dragan Huterer, Michael S. Turner
Recent use of Type Ia supernovae to measure acceleration of the universe has motivated questions regarding their optimal use to constrain cosmological parameters Omega_M, Omega_Λ a…
Kinematic Constraints to the Key Inflationary Observables
Mark B. Hoffman, Michael S. Turner
The observables and are key to testing and understanding inflation. (, , and respectively quantify the gravity-wave and density-perturbation contributions t…