Over the past five years two teams have used type Ia supernovae to trace the expansion of the Universe to a look back time more than 70% of the age of the Universe. These observations show an accelerating Universe which is best explained by a cosmological constant, or other form of dark energy with an equation of state near w=p/ρ=-1. There are many possible lurking systematic effects, and while difficult to completely eliminate, none of these appears large enough to challenge current results. However, as future experiments attempt to better characterize the equation of state of the matter leading to the observed acceleration, these systematic effects will ultimately limit progress
The discovery of cosmic acceleration is one of the most important developments in modern cosmology. ...
The primary agent for Type Ia supernova cosmology is the uniformity of their appearance. We present ...
Schwarz D, Kalus B, Seikel M. On the accelerated expansion of the cosmos. Prog.Part.Nucl.Phys. 2011;...
Over the past five years two teams have used type la supernovae to trace the expansion of the univer...
Over the past decade, supernovae have emerged as some of the most powerful tools for measuring extra...
The cause of the accelerating expansion of the universe has drawn much speculation in recent years. ...
The ‘standard’ model of cosmology is founded on the basis that the expansion rate of the universe is...
I review the use of Type Ia supernovae (SNe Ia) for cosmological distance determinations. Low-redshi...
It is generally argued that the present cosmological observations support the accelerating models of...
It is generally argued that present cosmological observations support the accelerating models of the...
Supernova observations show that the expansion of the universe has been speeding up. This unexpected...
In the late 1990’s, observations of two directionally-skewed samples of, in total, 93 Type Ia supern...
Seikel M, Schwarz D. How strong is the evidence for accelerated expansion? JOURNAL OF COSMOLOGY AND ...
The cosmological standard model at present is widely accepted as containing mainly things we do not ...
The fate of the Universe, infinite expansion or a big crunch , can be determined by measuring the r...
The discovery of cosmic acceleration is one of the most important developments in modern cosmology. ...
The primary agent for Type Ia supernova cosmology is the uniformity of their appearance. We present ...
Schwarz D, Kalus B, Seikel M. On the accelerated expansion of the cosmos. Prog.Part.Nucl.Phys. 2011;...
Over the past five years two teams have used type la supernovae to trace the expansion of the univer...
Over the past decade, supernovae have emerged as some of the most powerful tools for measuring extra...
The cause of the accelerating expansion of the universe has drawn much speculation in recent years. ...
The ‘standard’ model of cosmology is founded on the basis that the expansion rate of the universe is...
I review the use of Type Ia supernovae (SNe Ia) for cosmological distance determinations. Low-redshi...
It is generally argued that the present cosmological observations support the accelerating models of...
It is generally argued that present cosmological observations support the accelerating models of the...
Supernova observations show that the expansion of the universe has been speeding up. This unexpected...
In the late 1990’s, observations of two directionally-skewed samples of, in total, 93 Type Ia supern...
Seikel M, Schwarz D. How strong is the evidence for accelerated expansion? JOURNAL OF COSMOLOGY AND ...
The cosmological standard model at present is widely accepted as containing mainly things we do not ...
The fate of the Universe, infinite expansion or a big crunch , can be determined by measuring the r...
The discovery of cosmic acceleration is one of the most important developments in modern cosmology. ...
The primary agent for Type Ia supernova cosmology is the uniformity of their appearance. We present ...
Schwarz D, Kalus B, Seikel M. On the accelerated expansion of the cosmos. Prog.Part.Nucl.Phys. 2011;...