Results 231 to 240 of about 42,461 (272)

On the uncertainty principle of neural networks. [PDF]

iScience
Zhang JJ, Zhang DX, Chen JN, Pang LG, Meng D.   +4 more
europepmc   +1 more source

How intense is high-intensity interval training? Biomarker responses and associations with training load and fitness. [PDF]

iScience
Haller N, Widauer HL, Strepp T, Nunes N, Blumkaitis JC, Wenger M, Stöggl T, Aglas L.   +7 more
europepmc   +1 more source

Gravitational waves from slow combustion of a neutron star to quark star

, 2020
Shailendra Singh, Ritam Mallick, R. Prasad   +2 more
openalex   +1 more source

Centrality dependency of proton, deuteron, and triton's temperatures in Au+Au collisions at 200 GeV. [PDF]

Sci Rep
Khan I, Qudus A, Salouci M, Ismail AH.
europepmc   +1 more source

Inhibition of basal IL-6 activity promotes subcutaneous fat retention in humans during fasting and postprandial states. [PDF]

Cell Rep Med
Trinh B, Rasmussen SJ, Brøgger-Jensen ME, Engelhard CA, Lund A, Tavanez AR, Vassilieva A, Janum S, Iepsen UW, Kiens B, Møller K, Pedersen BK, Van Hall G, Ellingsgaard H.   +13 more
europepmc   +1 more source

Exercise capacity and cardiac allograft ischemic time in recent heart transplant recipients. [PDF]

JHLT Open
Bosteder KD, van Zyl JS, Arce-Esquivel AA, Cooper C, Felius J, Gottlieb RL.   +5 more
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

Quark star phenomenology

Physical Review D, 1978
We analyze models of quark matter appropriate to the description of matter at densities found within neutron stars. We consider in detail two models: quantum chromodynamics with a bag constant B = 56 MeV/fm/sup 3/, and quantum chromodynamics with B = 0.
Barry Freedman, Larry McLerran
openaire   +1 more source

Quark Matter in Neutron Stars

2020
Fil: Spinella, William M..
Spinella, William M., Weber, Fridolin, Contrera, Gustavo Aníbal Gabriel, Orsaria, Milva Gabriela   +3 more
openaire   +2 more sources

Stability of Quark Star Models

Communications in Theoretical Physics, 2016
Summary: In this paper, we investigate the stability of quark stars with four different types of inner matter configurations; isotropic, charged isotropic, anisotropic and charged anisotropic by using the concept of cracking. For this purpose, we have applied local density perturbations technique to the hydrostatic equilibrium equation as well as on ...
Azam, M., Mardan, S. A., Rehman, M. A.
openaire   +2 more sources

Quarks in stars

Soviet Physics Journal, 1974
The basic parameters — mass and radius — of the quark configurations having central densities from 1019 to 1032 g/cm3 are obtained. It is shown that similar objects should have large gravitational mass defects. The curve of the stable configurations is extended to the region of densities substantially exceeding those of the nucleus.
openaire   +1 more source