Session J6: Precision Measurements Impacting Cosmology

A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder

We report results from a program to determine the Hubble constant to $\sim$ 5\% precision from a refurbished distance ladder based on extensive use of differential measurements. The measurement makes use of 240 Cepheid variables observed with the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) on the {\it Hubble Space Telescope (HST)}. The Cepheids are distributed across six recent hosts of Type Ia supernovae (SNe~Ia) and the ``maser galaxy'' NGC 4258, allowing us to {\it directly} calibrate the peak luminosities of the SNe~Ia from the precise, geometric distance measurements provided by the masers. The homogeneity of the Cepheid periods and metallicities provided and our dependence on purely {\it differential} Cepheid fluxes enabled by the use of the same instruments for all Cepheid measurements reduces the largest systematic uncertainties in the determination of the fiducial SN Ia luminosity. In addition, the NICMOS measurements reduce the effects of differential extinction in the host galaxies by a factor of $\sim$5 over past optical data. Using the flux-redshift relation of SNe~Ia, we have measured $H_0$ with 4.7\% uncertainty including both statistical and systematic errors. We show that the factor of 2.2 improvement in the precision of $H_0$ is a significant aid to the determination of the equation-of-state parameter of dark energy, $w = P/(\rho c^2)$. Combined with the Wilkinson Microwave Anisotropy Probe 5-year measurements of $\Omega_M h^2$, we find $w= -1.12 \pm 0.12$, a result independent of high-redshift SNe~Ia and baryon acoustic oscillations (BAO), though consistent with their combination. The constraints on $w(z)$ now including high-redshift SNe~Ia and BAO are consistent with a cosmological constant and are improved by a factor of 3 due to the refinement in $H_0$ alone. We show that future improvements in the measurement of $H_0$ are likely and should further contribute to multi-technique studies of dark energy.   

Cosmology, scalar-tensor theories of gravity, and precision measurements at low energy

I review the scalar-tensor theories of gravity, their impact on cosmology, and discuss predictions for the high-precision measurements in laboratory and in space.   

Tests of Lorentz Invariance using Spinning Fermions and Laser Ranging to the Moon

Attempts to develop a quantum theory of gravity have focused attention on possible Planck-scale violations of Lorentz invariance. This talk will review recent experimental constraints on such violations obtained from laboratory experiments with polarized electrons or neutrons and from laser ranging to the moon.