Results 71 to 80 of about 669,527 (312)

Dark Energy and Tachyon Field in Bianchi Type-V Space-time [PDF]

open access: yesMod. Phys. Lett. A, Vol. 30, No. 1 (2015) 1550008, 2014
In this paper, we consider Bianchi type-V space-time and study a cosmological model of dark energy based on Tachyon scalar field. We assumed three different kinds of matter without possibility of interaction with scalar dark energy. Assuming power law Hubble parameter in terms of scale factor we obtain evolution of scalar field, scalar potential and ...
arxiv   +1 more source

Exploration of heterogeneity and recurrence signatures in hepatocellular carcinoma

open access: yesMolecular Oncology, EarlyView.
This study leveraged public datasets and integrative bioinformatic analysis to dissect malignant cell heterogeneity between relapsed and primary HCC, focusing on intercellular communication, differentiation status, metabolic activity, and transcriptomic profiles.
Wen‐Jing Wu   +15 more
wiley   +1 more source

Scalar Dark Matter Analysis of 6-Dimensional Effective Field Theory [PDF]

open access: yesarXiv, 2023
We give a prescription how high energy physics tools can be used to perform scalar dark matter analysis. We also present the analysis results of scalar dark matter in the context of 6 dimensional Effective Field Theory.
arxiv  

The atypical KRASQ22K mutation directs TGF‐β response towards partial epithelial‐to‐mesenchymal transition in patient‐derived colorectal cancer tumoroids

open access: yesMolecular Oncology, EarlyView.
TGF‐β has a complex role in cancer, exhibiting both tumor‐suppressive and tumor‐promoting properties. Using a series of differentiated tumoroids, derived from different stages and mutational background of colorectal cancer patients, we replicate this duality of TGF‐β in vitro. Notably, the atypical but highly aggressive KRASQ22K mutation rendered early‐
Theresia Mair   +17 more
wiley   +1 more source

Interacting Dark Energy in Hořava-Lifshitz Cosmology [PDF]

open access: yes, 2009
In the usual Ho\v{r}ava-Lifshitz cosmological models, the scalar field is responsible for dark matter. Using an additional scalar field, Saridakis \cite{sari} has formulated Ho\v{r}ava-Lifshitz cosmology with an effective dark energy sector. In the paper \cite{sari} the scalar fields do not interact with each other, here we extend this work to the ...
arxiv   +1 more source

Two-scalar-field model for the interaction of dark energy and dark matter [PDF]

open access: yesPhysical Review D, 2012
Version to match the one published in Physical Review D, 8 pages, 11 ...
Pedro Carrilho   +2 more
openaire   +3 more sources

Scalar dark matter induced oscillation of a permanent-magnet field

open access: yesPhysical Review D, 2023
9 pages, 1 ...
I. M. Bloch   +5 more
openaire   +4 more sources

Escape from TGF‐β‐induced senescence promotes aggressive hallmarks in epithelial hepatocellular carcinoma cells

open access: yesMolecular Oncology, EarlyView.
Chronic TGF‐β exposure drives epithelial HCC cells from a senescent state to a TGF‐β resistant mesenchymal phenotype. This transition is characterized by the loss of Smad3‐mediated signaling, escape from senescence, enhanced invasiveness and metastatic potential, and upregulation of key resistance modulators such as MARK1 and GRM8, ultimately promoting
Minenur Kalyoncu   +11 more
wiley   +1 more source

Baryogenesis via dark matter-induced symmetry breaking in the early Universe

open access: yesPhysics Letters B, 2017
We put forward a new proposal for generating the baryon asymmetry of the universe by making use of the dynamics of a U(1) scalar field coupled to dark matter.
Jeremy Sakstein, Mark Trodden
doaj   +1 more source

Irreversible thermodynamic description of interacting dark energy - dark matter cosmological models [PDF]

open access: yesPhys.Rev.D87:044018,2013, 2012
We investigate the interaction between dark energy and dark matter in the framework of irreversible thermodynamics of open systems with matter creation/annihilation. We consider dark energy and dark matter as an interacting two component (scalar field and "ordinary" dark matter) cosmological fluid in a homogeneous spatially flat and isotropic Friedmann-
arxiv   +1 more source

Home - About - Disclaimer - Privacy