Results 111 to 120 of about 41,644 (263)

Molecular responses in abdominal subcutaneous adipose tissue after a session of endurance exercise: effects of exercise intensity

The Journal of Physiology, EarlyView.
Abstract figure legend An acute session of aerobic exercise induces robust transcriptional changes in abdominal subcutaneous adipose tissue 1.5 h after exercise. Exercise at low‐, moderate‐ and high‐intensities each reveals some distinct molecular responses in adipose tissue.
Cheehoon Ahn, Tao Zhang, Thomas Rode, Gayoung Yang, Olivia K. Chugh, Sierra Ellis, Sophia Ghayur, Shriya Mehta, Ryan Salzman, Hui Jiang, Stephen C. J. Parker, Charles F. Burant, Jeffrey F. Horowitz   +12 more
wiley   +1 more source

Hadron-quark phase transition in the neutron star with vector MIT bag model and Korea-IBS-Daegu-SKKU functional

Frontiers in Astronomy and Space Sciences
Employing the Korea-IBS-Daegu-SKKU (KIDS) density functional for the hadron phase and the MIT bag model with vector (vBag) model for the quark phase, we obtain hadron-quark phase transition in neutron stars considering Maxwell construction.
Debashree Sen, Hana Gil, Chang Ho Hyun
doaj   +1 more source

Correlation Patterns of Muon Flux With Vertical Atmospheric Profiles: Insights From Monte Carlo Simulations

Journal of Geophysical Research: Space Physics, Volume 130, Issue 11, November 2025.
Abstract The production, attenuation, and absorption of secondary cosmic rays (SCR) are influenced by atmospheric parameters such as air pressure and temperature. To reliably correlate SCR flux measurements with atmospheric ionization driven by energetic particle precipitation, these dependencies must be quantified.
A. Al‐Qaaod, V. Pierrard, A. Winant, U. Stolzenberg, I. Ambrozova, M. Sommer, J. Slegl, J. Solc, A. Gkikoudi, A. G. Georgakilas, A. Papayannis, F. S. Krasniqi   +11 more
wiley   +1 more source

Neutron stars velocities and magnetic fields

EPJ Web of Conferences, 2018
We study a model that explain neutron stars velocities due to the anisotropic emission of neutrinos. Strong magnetic fields present in neutron stars are the source of the anisotropy in the system.
Paret Daryel Manreza, Martinez A. Perez, Ayala Alejandro., Piccinelli G., Sanchez A.   +4 more
doaj   +1 more source

Diquark condensation effects on hot quark star configurations

, 2004
The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation.We investigate the effects of a variation of the formfactors of the interaction on the phase diagram of quark matter.
A.M. Öztaş, Aguilera, Alford, Baldo, Bedaque, Berges, Blaschke, Blaschke, Blaschke, Blaschke, Blaschke, Blaschke, Carter, D. Blaschke, Frank, Fredriksson, Glendenning, Glendenning, Glendenning, Gocke, Grigorian, Grigorian, H. Grigorian, Hong, Horvath, Horvath, Huang, Iida, Jaikumar, Kastor, Kettner, Kiriyama, Lugones, Neumann, Oppenheimer, Ouyed, Page, Poghosyan, Prakash, Rajagopal, S. Fredriksson, Sahu, Schmidt, Sedrakian, Steiner   +44 more
core   +2 more sources

Setting sail for Paris 2024: Retrospective analysis of world‐class ILCA 7 Olympic sailors’ cardiorespiratory fitness (2015–2020)

Experimental Physiology, Volume 110, Issue 11, Page 1576-1583, November 1, 2025.
Abstract The aim of this retrospective analysis was to provide a more comprehensive understanding of the cardiorespiratory profile of world‐class ILCA‐7 sailors (n = 3, all males), through a longitudinal evaluation offering real‐world data on physiological profile and exercise intensity domains. The cardiopulmonary exercise testing (CPET) was performed
Damir Zubac, Zoran Valić, Vladimir Ivančev   +2 more
wiley   +1 more source

Quark stars in $$D_3$$ D 3 – $$D_7$$ D 7 holographic model

European Physical Journal C: Particles and Fields
This work investigates static and dynamical quark star properties within a $$D_3{-}D_7$$ D 3 - D 7 holographic model. We solve the Tolman–Oppenheimer–Volkoff equations for the quark matter equation of state obtained from the brane configuration.
M. Aleixo, C. H. Lenzi, W. de Paula, R. da Rocha   +3 more
doaj   +1 more source

Quark matter and quark stars at finite temperature in Nambu–Jona-Lasinio model

European Physical Journal C: Particles and Fields, 2017
We extend the SU(3) Nambu–Jona-Lasinio (NJL) model to include two types of vector interaction. Using these two types of vector interaction in NJL model, we study the quark symmetry free energy in asymmetric quark matter, the constituent quark mass, the ...
Peng-Cheng Chu, Xiao-Hua Li, Bin Wang, Yu-Min Dong, Yu-Yue Jia, Shu-Mei Wang, Hong-Yang Ma   +6 more
doaj   +1 more source

Rotating Quark Stars in General Relativity

Universe, 2018
We have built quasi-equilibrium models for uniformly rotating quark stars in general relativity. The conformal flatness approximation is employed and the Compact Object CALculator (cocal) code is extended to treat rotating stars with surface density ...
Enping Zhou, Antonios Tsokaros, Luciano Rezzolla, Renxin Xu, Kōji Uryū   +4 more
doaj   +1 more source

Phase Transition and Hybrid Star in a Nonlinear $\sigma - \omega$ model

, 1998
The phase transition between the nuclear matter and the quark matter is examined. The relativistic mean field theory(RMF) is consider with interacting nucleons and mesons using TM1 parameter set for the nuclear matter equations of state. It is found that
Blaizot D., Bogtrta A. E., L. MAHARANA, Mishra S. P., P. K. PANDA, R. MOHANTY, Remhard M, S. ACHARYA   +7 more
core   +1 more source