Star-Shaped Mesogens – Hekates: The Most Basic Star Structure with Three Branches

2011 ◽  
pp. 193-223 ◽  
Author(s):  
Matthias Lehmann
Keyword(s):  
Star Structure

Star structure connectivities of pancake graphs and burnt pancake graphs

2021 ◽  
pp. 1-9
Author(s):  
Subinur Dilixiati ◽  
Eminjan Sabir ◽  
Jixiang Meng
Keyword(s):  
Star Structure

Thin film poly-Si solar cell, with "star structure" on glass substrate fabricated at low temperature

2002 ◽  
Author(s):  
K. Yamamoto ◽  
M. Yoshimi ◽  
T. Suzuki ◽  
Y. Okamoto ◽  
Y. Tawada ◽  
...  
Keyword(s):  
Thin Film ◽  
Solar Cell ◽  
Low Temperature ◽  
Glass Substrate ◽  
Si Solar Cell ◽  
Star Structure

scholarly journals Neutron star structure in a quark model with excluded volume correction

2003 ◽  
Vol 68 (5) ◽  
Author(s):  
R. M. Aguirre ◽  
A. L. De Paoli
Keyword(s):  
Neutron Star ◽  
Quark Model ◽  
Excluded Volume ◽  
Volume Correction ◽  
Star Structure

scholarly journals Bounds on the speed of sound in dense matter, and neutron star structure

2017 ◽  
Vol 95 (4) ◽  
Author(s):  
Ch. C. Moustakidis ◽  
T. Gaitanos ◽  
Ch. Margaritis ◽  
G. A. Lalazissis
Keyword(s):  
Neutron Star ◽  
Speed Of Sound ◽  
Dense Matter ◽  
Star Structure

scholarly journals High-density QCD pairing in compact star structure

2003 ◽  
Vol 403 (1) ◽  
pp. 173-178 ◽  
Author(s):  
G. Lugones ◽  
J. E. Horvath
Keyword(s):  
Compact Star ◽  
High Density ◽  
Star Structure

Three-body forces and neutron star structure

2004 ◽  
Vol 69 (1) ◽  
Author(s):  
X. R. Zhou ◽  
G. F. Burgio ◽  
U. Lombardo ◽  
H.-J. Schulze ◽  
W. Zuo
Keyword(s):  
Neutron Star ◽  
Body Forces ◽  
Three Body ◽  
Star Structure

STRANGE STAR IN THE PRESENCE OF A STRONG MAGNETIC FIELD

2001 ◽  
Vol 16 (13) ◽  
pp. 2435-2445 ◽  
Author(s):  
P. K. SAHU ◽  
S. K. PATRA
Keyword(s):  
Magnetic Field ◽  
Strong Magnetic Field ◽  
Quark Matter ◽  
Strange Star ◽  
Structure Parameters ◽  
Strange Stars ◽  
Strange Matter ◽  
Free Quark ◽  
Star Structure

We study the effect of a strong magnetic field on interacting quark matter and apply the same to strange star. We find that interacting strange matter is less stable than noninteracting strange matter in the presence of a strong magnetic field. We then calculate strange star structure parameters such as mass and radius and find that the strange star is less compact for interacting quark matter than for free quark matter in presence of strong magnetic field. The maximum masses of strange stars are found to be within the recent observational limit.

scholarly journals The equation of state of dense matter and the effect of Λ hyperons to neutron star structure

2019 ◽  
Author(s):  
Stefano Gandolfi ◽  
Diego Lonardoni
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Dense Matter ◽  
Star Structure
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