ライフサイエンスコーパス: quark

1 s the decay of a beauty quark into a strange quark.

2 GPLv3 license at www.github.com/COMBINE-lab/quark.

3 nergy of about 130 MeV between the two charm quarks.

4 gly interacting and are therefore not 'free' quarks.

5 n terms of constructs made from two or three quarks.

6 We present Quark, a semi-reference-based compression tool designed

7 We demonstrate that Quark achieves state-of-the-art compression rates, and t

8 ately equal numbers of up, down, and strange quarks and are also called strangelets and nuclearites.

9 Here we investigate the dynamics of quarks and gluons inside nucleons using deeply virtual C

10 romodynamics to describe the interactions of quarks and gluons.

11 ees, it becomes a strongly coupled plasma of quarks and gluons.

12 , quantum chromodynamics (QCD) describes how quarks are bound inside hadrons by the strong force, med

13 ts on nonstandard neutrino interactions with quarks are derived from this initial data set.

14 can support a star this massive only if the quarks are strongly interacting and are therefore not 'f

15 y (approximately 280 MeV) between two bottom quarks (b) causes the analogous reaction with bottom qua

16 exothermic nature of the fusion of two heavy-quark baryons might manifest itself.

17 line was tested on 43 known sequences, where QUARK-based ab initio folding simulation generated model

18 ly charmed baryon , which contains two charm quarks (c) and one up quark (u) and has a mass of about

19 r-changing neutral current decays, whereby a quark changes its flavour without altering its electric

20 rovides an unambiguous constraint on strange quark contributions to the proton's magnetic moment thro

21 black holes in five dimensions has made the quark-gluon plasma an archetypical strongly coupled quan

22 stions about the structure and theory of the quark-gluon plasma are under active investigation.

23 ying star, and hydrodynamic transport of the quark-gluon plasma governed the expansion of the early U

24 uch as superconductors, neutron stars or the quark-gluon plasma of the early Universe, these gases ha

25 d laboratory plasmas, nuclear matter such as quark-gluon plasmas, electrons in solids, planetary core

26 Hypothetical Ca2+ "quarks" had little effect, as did blurring of sparks by

27 el variations such as an assumed first-order quark-hadron phase transition.

28 The possible alternate scenario of quark-hadron-induced inhomogeneities is also discussed.

29 en obtained that address the role of strange quarks in generating nuclear magnetism.

30 f such a transition is the decay of a beauty quark into a strange quark.

31 Quark is implemented in C ++11, and is available under a

32 Quarks, leptons, and three of the fundamental forces of

33 This reaction is a quark-level analogue of the deuterium-tritium nuclear fu

34 elease events amid noise: spontaneous Ca(2+) quark-like or "quarky" Ca(2+) release (QCR) events in ra

35 Quark makes use of a reference sequence when encoding re

36 evant to predictions of exotic new phases of quark matter and of strongly magnetized superconductors.

37 Quark matter can support a star this massive only if the

38 iterature, and conclude that the presence of quark matter in EXO 0748-676 is not ruled out.

39 utron star EXO 0748-676, Ozel concludes that quark matter probably does not exist in the centre of ne

40 such as hyperon-dominated matter, deconfined quark matter, superfluidity and superconductivity with c

41 mited set of possible equations of state for quark matter.

42 her densities because of a transformation to quark matter.

43 ased on a more comprehensive set of proposed quark-matter equations of state from the literature, and

44 scattering is expected to occur off a single quark, measurements show an intriguing sensitivity to gl

45 Inspired by the quark model by which composite particles (for example, p

46 ase) the TM-score (or RMSD) of the ab initio QUARK modeling by 12.1% (or 14.4%).

47 quark-nugget mass and to analyze testing the quark-nugget hypothesis for dark matter by observations

48 mpute the energy deposition as a function of quark-nugget mass and to analyze testing the quark-nugge

49 Quark nuggets are theoretical objects composed of approx

50 Previous efforts to detect quark nuggets assumed that the nuclear-density core inte

51 Tatsumi found that quark nuggets could well exist as a ferromagnetic liquid

52 and neutrons) are formed by combining three quarks (or flavours), here gold atoms are assigned three

53 hort lifetimes of the heavy bottom and charm quarks preclude any practical applications of such react

54 we report that this strong binding enables a quark-rearrangement, exothermic reaction in which two he

55 ment that are independent of the neutron and quark star's internal structure.

56 Neutron stars and quark stars are not only characterized by their mass and

57 ry inspirals, distinguish neutron stars from quark stars, and test general relativity in a nuclear st

58 Musings on mechanism: quest for a quark theory of proteins?

59 This allows Quark to achieve markedly better compression rates than

60 w hadrons constructed from increasingly many quarks to exist, just as atoms with increasing numbers o

61 mblies of interacting elements, ranging from Quarks to Galaxies, are at the heart of Physics.

62 b) causes the analogous reaction with bottom quarks () to have a much larger energy release of about

63 ich contains two charm quarks (c) and one up quark (u) and has a mass of about 3,621 megaelectronvolt

64 man-centered intuition as the confinement of quarks within protons or the event horizon of a black ho