Peebles (1989) showed that in the gravitational instability picture galaxy orbits can be traced back in time from a knowledge of their current positions, via a variational principle. We modify this variational principle so that galaxy redshifts can be input instead of distances, thereby recovering the distances. As a test problem, we apply the new method to a Local Group model. We infer M = 4 to 8 \Theta 10 12 M fi depending on cosmology, implying that the dynamics of the outlying Local Group dwarves are consistent with the timing argument. Some algorithmic issues need to be addressed before the method can be applied to recover nonlinear evolution from large redshift surveys, but there are no more difficulties in principle. Subject head...
We review the previous studies of galaxies and quasar redshifts discretisation. We present also the ...
Analysis of the peculiar velocities of galaxies should take account of the uncertainties in both red...
Aims. Redshift-space clustering anisotropies caused by cosmic peculiar velocities provide a powerful...
This dynamical model for the 28 galaxies with distances less than 1.5 Mpc, and not apparently tight ...
There is a ∼ 150 km s−1 discrepancy between the measured motion of the Local Group of galaxies (LG) ...
There is an ~150 km s-1 discrepancy between the measured motion of the Local Group (LG) of galaxies ...
The numerical action variational principle is used to find fully nonlinear solutions for the orbits ...
In this work we use the property that, on average, star formation rate increases with redshift for o...
This is the third paper in a series which combines N-body simulations and semi-analytic modelling to...
In the first paper in this series, a basic model was developed, for individual galaxies, consistin...
We present a precision study of large-scale structure from large galaxy redshift surveys. We focus o...
Ph.D. University of Hawaii at Manoa 2012.Includes bibliographical references.Studies at high redshif...
The changing universe model (CUM) describes galaxy parameter relationships (SESAPS '03, session EB 2...
We discuss the distribution of radial velocities of galaxies belonging to the Local Group. Two indep...
Reconstructing the density fluctuations in the early Universe that evolved into the distribution of ...
We review the previous studies of galaxies and quasar redshifts discretisation. We present also the ...
Analysis of the peculiar velocities of galaxies should take account of the uncertainties in both red...
Aims. Redshift-space clustering anisotropies caused by cosmic peculiar velocities provide a powerful...
This dynamical model for the 28 galaxies with distances less than 1.5 Mpc, and not apparently tight ...
There is a ∼ 150 km s−1 discrepancy between the measured motion of the Local Group of galaxies (LG) ...
There is an ~150 km s-1 discrepancy between the measured motion of the Local Group (LG) of galaxies ...
The numerical action variational principle is used to find fully nonlinear solutions for the orbits ...
In this work we use the property that, on average, star formation rate increases with redshift for o...
This is the third paper in a series which combines N-body simulations and semi-analytic modelling to...
In the first paper in this series, a basic model was developed, for individual galaxies, consistin...
We present a precision study of large-scale structure from large galaxy redshift surveys. We focus o...
Ph.D. University of Hawaii at Manoa 2012.Includes bibliographical references.Studies at high redshif...
The changing universe model (CUM) describes galaxy parameter relationships (SESAPS '03, session EB 2...
We discuss the distribution of radial velocities of galaxies belonging to the Local Group. Two indep...
Reconstructing the density fluctuations in the early Universe that evolved into the distribution of ...
We review the previous studies of galaxies and quasar redshifts discretisation. We present also the ...
Analysis of the peculiar velocities of galaxies should take account of the uncertainties in both red...
Aims. Redshift-space clustering anisotropies caused by cosmic peculiar velocities provide a powerful...