Discontinuity g ‐modes of hybrid stars: Effect of sequential phase transitions

2021 ◽  
Author(s):  
Maria Camila Rodríguez ◽  
Ignacio F. Ranea‐Sandoval ◽  
Mauro Mariani ◽  
Germán Malfatti ◽  
Octavio Miguel Guilera
Keyword(s):  
Phase Transitions ◽  
Hybrid Stars ◽  
Sequential Phase

scholarly journals Hybrid stars with sequential phase transitions: the emergence of the g2 mode

2021 ◽  
Vol 2021 (02) ◽  
pp. 009-009
Author(s):  
M.C. Rodríguez ◽  
Ignacio F. Ranea-Sandoval ◽  
M. Mariani ◽  
M. G. Orsaria ◽  
G. Malfatti ◽  
...  
Keyword(s):  
Phase Transitions ◽  
Hybrid Stars ◽  
Sequential Phase

Sequential Phase Transitions in Sm Substituted BiFeO$_{3}$

2011 ◽  
Vol 50 (9) ◽  
pp. 09NE08 ◽  
Author(s):  
Makoto Kubota ◽  
Kengo Oka ◽  
Yoshitaka Nakamura ◽  
Hisato Yabuta ◽  
Kaoru Miura ◽  
...  
Keyword(s):  
Phase Transitions ◽  
Sequential Phase

scholarly journals Sequential Phase Transitions in Sm Substituted BiFeO3

2012 ◽  
Vol 59 (5) ◽  
pp. 239-245
Author(s):  
Makoto Kubota ◽  
Kengo Oka ◽  
Yoshitaka Nakamura ◽  
Hisato Yabuta ◽  
Kaoru Miura ◽  
...  
Keyword(s):  
Phase Transitions ◽  
Sequential Phase

Sequential Phase Transitions with Switchable Dielectric Constant in a Metal-Free Ionic Crystal

2019 ◽  
Vol 2019 (19) ◽  
pp. 2443-2447 ◽  
Author(s):  
Jing Jing ◽  
Ji-Xing Gao ◽  
Guang-Meng Fan ◽  
Chao Shi ◽  
Zhi-Xin Gong ◽  
...  
Keyword(s):  
Dielectric Constant ◽  
Phase Transitions ◽  
Ionic Crystal ◽  
Metal Free ◽  
Sequential Phase

Sequential Phase Transitions in Sm Substituted BiFeO3

2011 ◽  
Vol 50 (9S2) ◽  
pp. 09NE08 ◽  
Author(s):  
Makoto Kubota ◽  
Kengo Oka ◽  
Yoshitaka Nakamura ◽  
Hisato Yabuta ◽  
Kaoru Miura ◽  
...  
Keyword(s):  
Phase Transitions ◽  
Sequential Phase

scholarly journals Quark-Hadron Hybrid Stars as Remnants of Supernovae Explosions

1999 ◽  
Vol 194 ◽  
pp. 327-329
Author(s):  
Gevorg S. Poghosyan
Keyword(s):  
Shock Wave ◽  
Phase Transitions ◽  
Time Scale ◽  
Free Fall ◽  
Central Density ◽  
Core Collapse ◽  
Hybrid Star ◽  
The Core ◽  
Hadron Phase ◽  
Hybrid Stars

It is expected that at explosion of Supernovae the mechanism of producing a shock wave is based on subatomic interactions, and the remnant of the supernovae explosion can be a hybrid quark-hadron star. Since the temperature in the centre of collapsing stars reaches of order T = 6 − 8 · 1010K and density electrons from the top of the Fermi sea can be captured and convert protons into neutrons via e− + p → n + ve. The capture of electrons results in a neutronization burst (V.S. Imshennik 1988). Core collapse of the progenitor star becomes essentially a free fall with a time scale . When the central density of the core reaches supernuclear densities the repulsive QCD forces becomes essential. This can bring about manifestations of quark-hadron phase transitions (A. Dar 1997). After the explosion, from the remaining matter is probably formed a hybrid star.

First-order phase transitions in rotating hybrid stars and pulsar glitches

2011 ◽  
Vol 11 (6) ◽  
pp. 679-686
Author(s):  
Fei Xiao ◽  
Chun-Mei Pi ◽  
Shu-Hua Yang ◽  
Ai-Zhi Zhou ◽  
Xiao-Ping Zheng
Keyword(s):  
Phase Transitions ◽  
First Order ◽  
Hybrid Stars ◽  
First Order Phase

Cooperative and Sequential Phase Transitions in it-Poly(propylene oxide)-b-poly(ethylene oxide)-b-it-poly(propylene oxide) Triblock Copolymers

2015 ◽  
Vol 48 (9) ◽  
pp. 3069-3079 ◽  
Author(s):  
Weichao Shi ◽  
Alaina J. McGrath ◽  
Youli Li ◽  
Nathaniel A. Lynd ◽  
Craig J. Hawker ◽  
...  
Keyword(s):  
Phase Transitions ◽  
Ethylene Oxide ◽  
Propylene Oxide ◽  
Triblock Copolymers ◽  
Poly Ethylene Oxide ◽  
Poly Ethylene ◽  
Poly Propylene ◽  
Sequential Phase
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