Results 251 to 260 of about 88,270 (291)

The Endocannabinoid-Microbiota-Neuroimmune Super-System: A Unifying Feedback Architecture for Systems Resilience, Collapse Trajectories, and Precision Feedback Medicine. [PDF]

Int J Mol Sci
Aliuș C, Breazu A, Pantu C, Toader C, Șerban M, Covache-Busuioc RA, Munteanu O, Dumitru AV.   +7 more
europepmc   +1 more source

A Faint Progenitor System for the Faint Supernova 2024vjm

Zimmerman E, Gal-Yam A, Groot P, Ofek E, Roestel Jv, Pastorello A, Valenti S, Ravi A, Chen P, Schulze S, Blagorodnova N, Wavasseur M, Gómez-Muñoz M, Tranin H, de Wet S, Leloudas G, Vreeswijk P, Kwok L, Schwab M, Jha S, Maguire K, Sand D, Stringer E, Kupfer T, Faran T, Anderson J, Andrews J, Andrews M, Badash A, Bloemen S, Bostroem K, Chen T, Valle MD, Dimitriadis G, Dong Y, Farah J, Gillanders J, Godson B, Gromadzki M, Hiramatsu D, Hoang E, Howell D, Janzen D, Kuncarayakti H, Li J, Lyman J, Maeda K, Magee M, Mehta D, Milligan A, Moran S, Ni YQ, O’Neill D, Pearson J, Pieterse D, Pignata G, Reguitti A, Reichart D, Retamal NM, Santos R, Scaringi S, Shrestha M, Srivastav S, Stoppa F, Subrayan B, Valerin G, Wang X, Wynn K, Yaron O, Zang W.   +69 more
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Baryon number creation and phase transitions in the early universe

, 1982
Hut, P., Klinkhamer, F.R.
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Ultrarelativistic Phase Transition in the early Universe: The faster the better

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Phase transitions in the early universe

La Rivista Del Nuovo Cimento Series 3, 1986
On passe en revue les resultats recents obtenus dans les principaux domaines ou la recherche cosmologique et la physique des interactions fondamentales se ...
S. A. Bonometto, A. Masiero
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Phase transitions and formation of bubbles in the early Universe

Physical Review D, 1992
We analyze the bubble-formation process that occurs when there is phase coexistence in the early Universe. In this paper we stress the relevance of determining the surface tension in order to compute some quantities that are relevent to cosmology such as the number density of bubbles, the contrast density, and the most probable sizes of bubbles ...
, Marques, , Ramos
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Invisible axions and the QCD phase transition in the early Universe

Physical Review D, 1986
We examine, in detail, the conditions under which the quark-hadron phase transition in the early Universe can influence the previously determined upper bound on the axion decay constant f/sub a/< or approx. =5 x 10/sup 12/ GeV. By integrating the axion equation of motion (in general and in a specific model) through the phase transition we find that if ...
, DeGrand, , Kephart, , Weiler
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Phase transition of the two Higgs doublets in early universe

International Journal of Modern Physics A, 2023
In this paper, we study the phase transition of the two Higgs-doublets model (2HDM) and consider a scenario of a electroweak phase transition at alignment limit. Using the Cornwall–Jackiw–Tomboulis formalism at finite temperature, we consider the phase transition of the aligned 2HDM in the two-loop double-bubble contribution.
Nguyen Tuan Anh, Dinh Thanh Tam
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NONEQUILIBRIUM PHASE TRANSITIONS IN THE EARLY UNIVERSE

Particles and the Universe, 2004
We review the current issues of nonequilibrium phase transitions, in particular, in the early Universe. Phase transitions cannot maintain thermal equilibrium and become nonequilibrium when the thermal relaxation time scale is bigger than the dynamical time scale.
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Modeling a delayed phase transition in the early universe

Journal of Physics G: Nuclear and Particle Physics, 2014
We use an effective field-theoretical model to describe a QCD-type phase transition in the early universe. It is assumed that the formation of a new phase proceeds via supercooling and thermal activation. A subsequent rolling-down process is characterized by a microscopic time scale of a few .
Daniel Yueker, Igor Mishustin, Marcus Bleicher   +2 more
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