Journal ArticleDOI
The early universe
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The early Universe, at times prior to recombination 10 5.5 years after the Big Bang, can not be studied by looking at individual objects as discussed by the authors, but there are several fossils from this epoch that can be studied.About:
This article is published in Advances in Space Research.The article was published on 2000-06-01. It has received 33 citations till now. The article focuses on the topics: Age of the universe & Observable universe.read more
Citations
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A Relation Between Distance and Radial Velocity Among Extra-Galactic Nebulae
TL;DR: In this article, a re-examination of the relationship between apparent radial velocities and distances is presented, based on only those nebular distances which are believed to be fairly reliable.
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Cosmological Implications of Quantum Anomalies
TL;DR: Barrie et al. as mentioned in this paper investigated the possible implications of quantum anomalies in the early universe, and proposed a new mechanism for cogenesis during inflation, in which a new anomalous U(1)X gauge group was introduced.
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Higgs Effective Field Theories - Systematics and Applications
TL;DR: In this paper, effective field theories (EFTs) for the Higgs particle, which is not necessarily a Higgs of the Standard Model, are discussed for decoupling and non-decoupling.
Phenomenological study of the minimal r-symmetric supersymmetric standard model
TL;DR: In this article, a minimal R-symmetric supersymmetric extension of the standard model of particle physics (MSSM) is studied and its effects on the parameters of the MRSSM are investigated.
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Modified Theories of Gravity
TL;DR: In this article, the authors consider two different models, the Cascading DGP and the dRGT massive gravity, which are candidates for viable models to modify gravity at very large distances.
References
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Journal ArticleDOI
Inflationary universe: A possible solution to the horizon and flatness problems
TL;DR: In this paper, the authors proposed a model of hot big-bang cosmology where the early universe is assumed to be highly homogeneous, in spite of the fact that separated regions were causally disconnected (horizon problem).
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A new type of isotropic cosmological models without singularity
TL;DR: In this paper, the Einstein equations with quantum one-loop contributions of conformally covariant matter fields are shown to admit a class of nonsingular isotropic homogeneous solutions that correspond to a picture of the universe being initially in the most symmetric (de Sitter) state.
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Synthesis of the Elements in Stars
TL;DR: In this article, a count of the stable and radioactive elements and isotopes is given, and Table I,1 shows that only promethium has not been found in nature, whereas 99 elements are found terrestrially and technetium is found in stars.
A Relation Between Distance and Radial Velocity among Extragalactic Nebulae
TL;DR: A re-examination of the question of the motion of the sun with respect to the extra-galactic nebulae, based on only those nebular distances which are believed to be fairly reliable, indicates the probability of an approximately uniform upper limit to the absolute luminosity of stars, in the late-type spirals and irregular neBulae at least.
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The Cosmic Microwave Background spectrum from the full COBE FIRAS data set
TL;DR: In this article, the Far-InfraRed Absolute Spectrophotometer (FIRAS) on board the COBE (COsmic Background Explorer) is used to measure the difference between the cosmic microwave background and a precise blackbody spectrum.