Results 81 to 90 of about 1,005 (182)
In this paper, we investigate the validity of the so-called cosmic no-hair conjecture in the framework of anisotropic inflation models of non-canonical scalar fields non-minimally coupled to a two-form field.
Tuyen M. Pham +3 more
doaj +1 more source
Responsive liquid metal materials towards unstructured environment
Room‐temperature liquid metals integrate conductivity, deformability, and interfacial dynamics, enabling robust performance in unstructured environments. This review highlights key properties, requirements, and applications across in vivo, underwater, natural, space, and radiation settings, with advances in sensing, actuation, thermal regulation, and ...
Bo Yuan +5 more
wiley +1 more source
Testing inflation with the cosmic microwave background
(differs from original inclusion of color version of figure 3 and corrected version of figure 2), 11 pages plus 4 figures (attached as a uuencoded postscript file), LaTeX, FNAL--PUB--94/053 ...
Dodelson, Scott +2 more
openaire +3 more sources
Plant pathogens worldwide continue to spread outside of their native ranges into new habitats. Our results highlight the importance of investigating variable processes like land use legacy that can correlate with impacts of non‐native plant pathogens.
Kristy Stevenson +5 more
wiley +1 more source
Proposed physical mechanism that gives rise to cosmic inflation. [PDF]
Law BM.
europepmc +1 more source
Cosmic microwave background probes models of inflation
Inflation creates both scalar (density) and tensor (gravity wave) metric perturbations. We find that the tensor mode contribution to the CMB anisotropy on large-angular scales can only exceed that of the scalar mode in models where the spectrum of perturbations deviates significantly from scale invariance (e.g., extended and power-law inflation models ...
Davis, Richard Lynn +4 more
openaire +4 more sources
Simple cosmological model with inflation and late times acceleration
In the framework of polynomial Palatini cosmology, we investigate a simple cosmological homogeneous and isotropic model with matter in the Einstein frame.
Marek Szydłowski, Aleksander Stachowski
doaj +1 more source
Intermediate Inflation or Late Time Acceleration?
The expansion rate of “intermediate inflation” lies between the exponential and power law expansion but corresponding accelerated expansion does not start at the onset of cosmological evolution.
Abhik Kumar Sanyal
doaj +1 more source
T-model Higgs inflation and metastable cosmic strings
We present the formation of metastable cosmic strings (CSs) in the context of a supersymmetric (SUSY) left-right model. The spontaneous SU(2)R symmetry breaking occurs during a stage of T-model (Higgs) inflation (TI) driven by an SU(2)R triplet ...
C. Pallis
doaj +1 more source
Why concave rather than convex inflaton potential?
The Planck data on cosmic microwave background indicates that the Starobinsky-type model with concave inflation potential is favored over the convex-type chaotic inflation. Is there any reason for that?
Pisin Chen, Dong-han Yeom
doaj +1 more source

