The energy conditions give upper bounds on the luminosity distance. We apply these upper bounds to the 192 essence supernova Ia data to show that the Universe had experienced accelerated expansion. This conclusion is drawn directly from the distance modulus-reshift graph. In addition to be a very simple method, this method is also totally independent of any cosmological model. From the degeneracy of the distance modulus at low redshift, we argue that the choice of $w_0$ for probing the property of dark energy is misleading. One explicit example is used to support this argument
Distance-redshift diagrams probe expansion history of the Universe. We show that the stellar mass-bi...
Understanding the acceleration of the universe and its cause is one of the key problems in physics a...
The High-z Supernova Search Team has discovered and observed 8 new supernovae in the redshift interv...
The comparison of redshift-distance relationship for high and low-redshift supernovae revealed the s...
Supernovae searches have been been suggested as a method for determining precisely the current value...
Understanding the acceleration of the universe and its cause is one of the key problems in physics a...
We extend and apply a model-independent analysis method developed earlier by Daly & Djorgovski to ne...
A major recent evelopment in observational cosmology has been an accurate measurement of the luminos...
The supernovae Hubble diagram traces the expansion history of the universe, including the influence ...
Currently available Type Ia distant supernovae observed data seem to support evidence that the cosmi...
AbstractWe test if the latest Gold set of 182 SNIa or the combined “Platinum” set of 192 SNIa from t...
Understanding the nature of dark energy, which appears to drive the expansion of the universe, is on...
Determination of the expansion and acceleration history of the universe is one of the fundamental go...
The luminosity distance-redshift relation is one of the fundamental tools of modern cosmology. We co...
We test if the latest Gold set of 182 SNIa in conjunction with the CMB shift parameter show a prefer...
Distance-redshift diagrams probe expansion history of the Universe. We show that the stellar mass-bi...
Understanding the acceleration of the universe and its cause is one of the key problems in physics a...
The High-z Supernova Search Team has discovered and observed 8 new supernovae in the redshift interv...
The comparison of redshift-distance relationship for high and low-redshift supernovae revealed the s...
Supernovae searches have been been suggested as a method for determining precisely the current value...
Understanding the acceleration of the universe and its cause is one of the key problems in physics a...
We extend and apply a model-independent analysis method developed earlier by Daly & Djorgovski to ne...
A major recent evelopment in observational cosmology has been an accurate measurement of the luminos...
The supernovae Hubble diagram traces the expansion history of the universe, including the influence ...
Currently available Type Ia distant supernovae observed data seem to support evidence that the cosmi...
AbstractWe test if the latest Gold set of 182 SNIa or the combined “Platinum” set of 192 SNIa from t...
Understanding the nature of dark energy, which appears to drive the expansion of the universe, is on...
Determination of the expansion and acceleration history of the universe is one of the fundamental go...
The luminosity distance-redshift relation is one of the fundamental tools of modern cosmology. We co...
We test if the latest Gold set of 182 SNIa in conjunction with the CMB shift parameter show a prefer...
Distance-redshift diagrams probe expansion history of the Universe. We show that the stellar mass-bi...
Understanding the acceleration of the universe and its cause is one of the key problems in physics a...
The High-z Supernova Search Team has discovered and observed 8 new supernovae in the redshift interv...