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1 ich was 2.6 times more than that achieved by QUARK.
2 s the decay of a beauty quark into a strange quark.
3 ydrodynamic flow of electrons, neutrons, and quarks.
4 nergy of about 130 MeV between the two charm quarks.
5 gly interacting and are therefore not 'free' quarks.
6 ately equal numbers of up, down, and strange quarks.
7 n terms of constructs made from two or three quarks.
8 ound in quantum chromodynamics (QCD) between quarks.
9 s, with the Cooper pairs playing the role of quarks.
10 iated blips, and ryanodine receptor mediated quarks.
11 fir 79.69 +/- 6.51 %, skyr 78.12 +/- 5.22 %, quark 65.37 +/- 4.72 %).
12                                   We apply C-QUARK, a deep-learning contact-guided ab initio structur
13                                   We present Quark, a semi-reference-based compression tool designed
14 sitively- (up) and negatively-charged (down) quarks, a result of the complex quark-gluon dynamics, le
15                          We demonstrate that Quark achieves state-of-the-art compression rates, and t
16 strong interaction that binds its elementary quark and gluon constituents.
17 ately equal numbers of up, down, and strange quarks and are also called strangelets and nuclearites.
18  stems from fundamental interactions between quarks and gluons (the constituents of nucleons) that ar
19          Here we investigate the dynamics of quarks and gluons inside nucleons using deeply virtual C
20 lex dynamics of its fundamental constituents-quarks and gluons-described by the theory of quantum chr
21 he fundamental building blocks of the proton-quarks and gluons-have been known for decades.
22 ned quark matter, liberating its constituent quarks and gluons.
23 romodynamics to describe the interactions of quarks and gluons.
24 ees, it becomes a strongly coupled plasma of quarks and gluons.
25  nuclear physics, the neutrino conversion to quarks and hadrons is based on gravitational forces, com
26 e meV/c(2) range and reach the mass range of quarks and hadrons, i.e. the GeV/c(2) range.
27 heir being composed of strange, up, and down quarks and have not included any effects caused by their
28                                   The two up quarks and the single down quark that comprise the proto
29 ncrease in their masses which reach those of quarks, and a concomitant dramatic relativistic increase
30                           In this picture of quark-antiquark creation by the strong force, the probab
31                                         When quark-antiquark pairs are separated, the energy stored i
32 , quantum chromodynamics (QCD) describes how quarks are bound inside hadrons by the strong force, med
33 ts on nonstandard neutrino interactions with quarks are derived from this initial data set.
34  can support a star this massive only if the quarks are strongly interacting and are therefore not 'f
35 y (approximately 280 MeV) between two bottom quarks (b) causes the analogous reaction with bottom qua
36 exothermic nature of the fusion of two heavy-quark baryons might manifest itself.
37 line was tested on 43 known sequences, where QUARK-based ab initio folding simulation generated model
38 ly charmed baryon , which contains two charm quarks (c) and one up quark (u) and has a mass of about
39 r-changing neutral current decays, whereby a quark changes its flavour without altering its electric
40 ent of spinons, a condensed matter analog of quark confinement in quantum chromodynamics.
41 which exhibit non-perturbative effects like 'quark confinement' and 'false vacuum decay'.
42 rovides an unambiguous constraint on strange quark contributions to the proton's magnetic moment thro
43 tact accuracy or few homologous sequences, C-QUARK correctly folded 6 times more proteins than other
44 ested on 247 non-redundant proteins, where C-QUARK could fold 75% of the cases with TM-scores (templa
45 o particle physics examples, Z-boson and top-quark decays, but stress that OTUS can be widely applied
46 arged (down) quarks, a result of the complex quark-gluon dynamics, lead to a negative value for its s
47 rotation and is expected to occur in the hot quark-gluon fluid (the "subatomic swirl") created in rel
48 hese little bangs of transient collisions, a quark-gluon plasma (QGP) of nearly vanishing viscosity i
49  black holes in five dimensions has made the quark-gluon plasma an archetypical strongly coupled quan
50 stions about the structure and theory of the quark-gluon plasma are under active investigation.
51 ying star, and hydrodynamic transport of the quark-gluon plasma governed the expansion of the early U
52 uch as superconductors, neutron stars or the quark-gluon plasma of the early Universe, these gases ha
53 uark nuggets (MQNs) after formation from the quark-gluon plasma until expansion of the universe freez
54 d laboratory plasmas, nuclear matter such as quark-gluon plasmas, electrons in solids, planetary core
55                           Hypothetical Ca2+ "quarks" had little effect, as did blurring of sparks by
56 el variations such as an assumed first-order quark-hadron phase transition.
57           The possible alternate scenario of quark-hadron-induced inhomogeneities is also discussed.
58  spin of protons, which are shared among the quarks, have been investigated previously using electron
59 en obtained that address the role of strange quarks in generating nuclear magnetism.
60 ple is confinement, responsible for bounding quarks inside hadrons such as protons or neutrons(1).
61 f such a transition is the decay of a beauty quark into a strange quark.
62 on mass, the bulk of which is in the form of quark kinetic and potential energy and gluon energy from
63                                              Quarks, leptons, and three of the fundamental forces of
64                           This reaction is a quark-level analogue of the deuterium-tritium nuclear fu
65 elease events amid noise: spontaneous Ca(2+) quark-like or "quarky" Ca(2+) release (QCR) events in ra
66                                              Quark makes use of a reference sequence when encoding re
67 evant to predictions of exotic new phases of quark matter and of strongly magnetized superconductors.
68                                              Quark matter can support a star this massive only if the
69                                              Quark matter exhibits an approximate conformal symmetry,
70 iterature, and conclude that the presence of quark matter in EXO 0748-676 is not ruled out.
71 utron star EXO 0748-676, Ozel concludes that quark matter probably does not exist in the centre of ne
72 n where nuclear matter melts into deconfined quark matter, liberating its constituent quarks and gluo
73 such as hyperon-dominated matter, deconfined quark matter, superfluidity and superconductivity with c
74 ly massive stars, the EoS is consistent with quark matter.
75 mited set of possible equations of state for quark matter.
76 her densities because of a transformation to quark matter.
77 ased on a more comprehensive set of proposed quark-matter equations of state from the literature, and
78 scattering is expected to occur off a single quark, measurements show an intriguing sensitivity to gl
79                              Inspired by the quark model by which composite particles (for example, p
80 ase) the TM-score (or RMSD) of the ab initio QUARK modeling by 12.1% (or 14.4%).
81 nd that the core of a magnetar star may be a quark nugget in a ferromagnetic state with core magnetic
82                 We apply Tatsumi's result to quark-nugget dark-matter and report results on aggregati
83 quark-nugget mass and to analyze testing the quark-nugget hypothesis for dark matter by observations
84 mpute the energy deposition as a function of quark-nugget mass and to analyze testing the quark-nugge
85                      A search for magnetised quark nuggets (MQN) is reported using acoustic signals f
86  report results on aggregation of magnetized quark nuggets (MQNs) after formation from the quark-gluo
87                                              Quark nuggets are a candidate for dark matter consistent
88                                              Quark nuggets are a candidate for dark matter, which has
89                                              Quark nuggets are theoretical objects composed of approx
90                                              Quark nuggets are theoretical objects composed of approx
91                   Previous efforts to detect quark nuggets assumed that the nuclear-density core inte
92                           Tatsumi found that quark nuggets could well exist as a ferromagnetic liquid
93                      Most previous models of quark nuggets have assumed no intrinsic magnetic field;
94                           Previous models of quark nuggets have investigated properties arising from
95  magnetic field; however, Tatsumi found that quark nuggets may exist in magnetars as a ferromagnetic
96                      We apply that result to quark nuggets, a dark-matter candidate consistent with t
97  and neutrons) are formed by combining three quarks (or flavours), here gold atoms are assigned three
98 nt down antimatter quarks than up antimatter quarks over a wide range of momenta.
99 le in reactions in which a matter-antimatter quark pair annihilates.
100 , is its ability to create matter-antimatter quark pairs inside the proton that exist only for a very
101 isospin symmetry between up (u) and down (d) quarks, part of the more general flavor symmetry.
102 hort lifetimes of the heavy bottom and charm quarks preclude any practical applications of such react
103  and ambient neutrinos for the generation of quarks, protons and neutrons, i.e. for the generation of
104 ate-of-the-art full-version methods, namely, Quark, RaptorX, Rosetta, MULTICOM and trRosetta in the C
105 we report that this strong binding enables a quark-rearrangement, exothermic reaction in which two he
106 m for the presence of up and down antimatter quarks should be nearly identical, given that their mass
107 ment that are independent of the neutron and quark star's internal structure.
108                            Neutron stars and quark stars are not only characterized by their mass and
109 ry inspirals, distinguish neutron stars from quark stars, and test general relativity in a nuclear st
110 ifferent, with more abundant down antimatter quarks than up antimatter quarks over a wide range of mo
111        The two up quarks and the single down quark that comprise the proton in the simplest picture a
112               Here, we developed a method, C-QUARK, that integrates multiple deep-learning and coevol
113            Musings on mechanism: quest for a quark theory of proteins?
114                                  This allows Quark to achieve markedly better compression rates than
115 w hadrons constructed from increasingly many quarks to exist, just as atoms with increasing numbers o
116 mblies of interacting elements, ranging from Quarks to Galaxies, are at the heart of Physics.
117 b) causes the analogous reaction with bottom quarks () to have a much larger energy release of about
118 ich contains two charm quarks (c) and one up quark (u) and has a mass of about 3,621 megaelectronvolt
119                                            C-QUARK was also tested on 64 free-modeling targets from t
120 heir fleeting existence makes the antimatter quarks within protons difficult to study, but their exis
121 man-centered intuition as the confinement of quarks within protons or the event horizon of a black ho

 
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