The case for a positive cosmological Λ-term
Recent observations of Type 1a supernovae indicating an accelerating universe have once
more drawn attention to the possible existence, at the present epoch, of a small positive Λ …
more drawn attention to the possible existence, at the present epoch, of a small positive Λ …
The cosmic triangle: Revealing the state of the universe
The cosmic triangle is introduced as a way of representing the past, present, and future
status of the universe. Our current location within the cosmic triangle is determined by the …
status of the universe. Our current location within the cosmic triangle is determined by the …
Measurements of Ω and Λ from 42 high-redshift supernovae
S Perlmutter, G Aldering, G Goldhaber… - The Astrophysical …, 1999 - iopscience.iop.org
We report measurements of the mass density, Ω $\mathstrut {_ {M}} $, and cosmological-
constant energy density, Ω $\mathstrut {_ {{\Lambda}}} $, of the universe based on the …
constant energy density, Ω $\mathstrut {_ {{\Lambda}}} $, of the universe based on the …
Observational evidence from supernovae for an accelerating universe and a cosmological constant
We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the
redshift range 0.16≤ z≤ 0.62. The luminosity distances of these objects are determined by …
redshift range 0.16≤ z≤ 0.62. The luminosity distances of these objects are determined by …
Final results from the Hubble Space Telescope key project to measure the Hubble constant
WL Freedman, BF Madore, BK Gibson… - The Astrophysical …, 2001 - iopscience.iop.org
We present here the final results of the Hubble Space Telescope (HST) Key Project to
measure the Hubble constant. We summarize our method, the results, and the uncertainties …
measure the Hubble constant. We summarize our method, the results, and the uncertainties …
Curvature quintessence
S Capozziello - International Journal of Modern Physics D, 2002 - World Scientific
The issues of quintessence and cosmic acceleration can be discussed in the framework of
higher order theories of gravity. We can define effective pressure and energy density directly …
higher order theories of gravity. We can define effective pressure and energy density directly …
Non-baryonic dark matter: observational evidence anddetection methods
L Bergström - Reports on Progress in Physics, 2000 - iopscience.iop.org
The evidence for the existence of dark matter in the universe is reviewed. A general picture
emerges, where both baryonic and non-baryonic dark matter is needed to explain current …
emerges, where both baryonic and non-baryonic dark matter is needed to explain current …
Quintessence without scalar fields
The issues of quintessence and cosmic acceleration can be discussed in the framework of
theories which do not include necessarily scalar fields. It is possible to define pressure and …
theories which do not include necessarily scalar fields. It is possible to define pressure and …
Toward better age estimates for stellar populations: the Y2 isochrones for solar mixture
We have constructed a new set of isochrones, called the Y 2 Isochrones, that represent an
update of the Revised Yale Isochrones (RYI), using improved opacities and equations of …
update of the Revised Yale Isochrones (RYI), using improved opacities and equations of …
[BOOK][B] Science and the Akashic field: An integral theory of everything
E Laszlo - 2007 - books.google.com
Presents the unifying world-concept long sought by scientists, mystics, and sages: an
Integral Theory of Everything• Explains how modern science has rediscovered the Akashic …
Integral Theory of Everything• Explains how modern science has rediscovered the Akashic …