Results 151 to 160 of about 708 (181)

Developing a hybrid technique for energy demand forecasting based on optimized improved SVM by the boosted multi-verse optimizer: Investigation on affecting factors. [PDF]

Heliyon
Huang A, Bi Q, Dai L, Hosseinzadeh H.
europepmc   +1 more source

Enhancing breast cancer diagnosis using deep learning and gradient multi-verse optimizer: a robust biomedical data analysis approach. [PDF]

PeerJ Comput Sci
El Kati Y, Wang SL, Taresh MM, Ali TAA.
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Overview of the ESCAPE Dark Matter Test Science Project for astronomers. [PDF]

Open Res Eur
Pearson J, Dickinson H, Sinha S, Serjeant S.   +3 more
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Practitioner perspectives on extended difficulties and optimal support strategies following psychedelic experiences: a qualitative analysis. [PDF]

Harm Reduct J
Argyri EK, Krecké J, Robinson OC, Evans J, Skragge M, Morgan CJA.   +5 more
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Leptogenesis with perturbations in type-II and type-III seesaw models. [PDF]

Eur Phys J C Part Fields
Baldes I.
europepmc   +1 more source

The particle-gravity frontier. [PDF]

Philos Trans A Math Phys Eng Sci
Bass SD, Harz J, Heisenberg L.
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Inflation in inhomogeneous cosmology

Physical Review D, 1992
We discuss the onset of inflation in an inhomogeneous, asymptotically Friedmann-Robertson-Walker universe coupled to a scalar inflaton field. We consider a three-parameter family of inhomogeneous Cauchy data, for which we can solve analytically the constraint equations.
, Calzetta, , Sakellariadou
openaire   +2 more sources

Inflation and quantum cosmology

Physica Scripta, 1990
Contents: 1. Introduction; 2. Chaotic inflation; 3. Self-reproducing inflationary universe; 4. Adjusting to the new paradigm: absence of cosmological constraints on the axion mass in the inflationary cosmology; 5. Inflation and the wave function of the universe; 6. Chaotic inflation versus extended inflation; 7. Stochastic approach to the baby universe
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Inflation and the decaying cosmological constant

Physical Review D, 1992
The interaction of a Higgs field incorporated in the model of a decaying cosmological constant is discussed. This interaction is shown to provide a promising mechanism for sufficient reheating following inflation.
, Nishioka, , Fujii
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Inflation and cosmological perturbations

1996
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
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