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Dark Matter and Dark Energy
Dark Matter and Dark Energy

... Particle is a superpartner of a gauge boson in most models: “bino” a perfect candidate for WIMP • But there are many other possibilities (technibaryons, gravitino, axino, invisible axion, WIMPZILLAS, etc) ...
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Slide 1

... An overview of the advanced accelerator research at SLAC. Experiments are being conducted with the goal of exploring high gradient acceleration mechanisms. One line of research is devoted to plasma wakefield acceleration where a plasma wave is excited by a beam. Particles in the head of the beam los ...
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H-modeCoreEdgeSOL_TIJSAT1_rev1
H-modeCoreEdgeSOL_TIJSAT1_rev1

... density of the main plasma region. To solve for the flow of material entering the scrapeoff into a high-recycling region, the model ignores all radial flows in the scrape-off and considers only parallel flow along the field lines. The fluid equations, including sources, have been derived in arbitrar ...
Introduction to Statistical Issues in Particle Physics - SLAC
Introduction to Statistical Issues in Particle Physics - SLAC

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Elementary Particles in Physics

... deep principle that makes baryon conservation compelling, and it may turn out that baryon conservation is only approximate. The particles with integer spin are called mesons, and they have baryon number B = 0. There are hundreds of different kinds of hadrons, some almost stable and some (known as re ...
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HIC: ALICE, The Wonderland more or less personal view

Neutron star to strange star - Institute of Physics, Bhubaneswar
Neutron star to strange star - Institute of Physics, Bhubaneswar

... radius could give a clear picture of the EOS of pulsars, and thereby establish them as NS and/or QS. Is it possible ? If not, the theorist have to come up with other models whose observable should be able to distinguish compact stars. New detectors with more accurate observations, one expects to mea ...
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... takes place through a series of two-body reactions, building more massive nuclei step by step. The essential first step is the fusion of a proton and a neutron to synthesize a deuterium nucleus: p+n↔D+γ . (Compare with the equation that describes recombination: p + e− ↔ H + γ .) The energy released ...
Resonances and Excited States
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... Particles that are unstable against decay by the strong interaction have mean lives of the order of 10 23 s and therefore cannot be detected by ordinary means. For example, if such a particle moves with nearly the speed of light, it can travel a distance of only about r = c" = 13 * 108 m>s2 110-23 s ...
Kinetic Studies of Nonrelativistic Young Supernova Remnant
Kinetic Studies of Nonrelativistic Young Supernova Remnant

... lead to stronger magnetic fields downstream of the forward shocks, rather than reverse shocks. We would thus expect synchrotron emission to originate from the magnetized structure of the forward shock transition, which is in agreement with SNR observations. We have also studied the effect of the ass ...
Historical Perspective
Historical Perspective

The Universe - The Ohio State University
The Universe - The Ohio State University

... forces. Nuclear forces were then able to pull two up quarks and one down quark together to form a proton, and two down quarks and one up quark to form a neutron. Protons and neutrons are referred to as nucleons. Baryons also refer to protons and neutrons. Particles were at random motions at relativi ...
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How does one probe dense matter at 1012 K ?

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Synchrotron - schoolphysics

... The Proton Synchrotron at CERN in Geneva has an orbit diameter of 172m, deflecting magnets of 1.4T and accelerates protons to 28 GeV. Each proton pulse contains about 1011 protons and during the acceleration the protons travel some 80 000 km (50 000 miles)! Protons from the synchrotron are shot into ...
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Chapter 30: Nuclear Physics
Chapter 30: Nuclear Physics

... the number that remain undecayed at the end of time t is given by N = N0e-t/τ = N0(½) t/τ . The time constant τ is related to the half-life t1/2: t1/2 = τ ln2= 0.693τ. The activity is then given by R = R0e-t/τ = R0(½) t/τ where R0 is the activity at t = 0. ...
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... • Has binding energies that are small compared to their rest masses • Has non-relativistic internal velocities ...
ICHEP_2010_Electroweak_Stars
ICHEP_2010_Electroweak_Stars

... Can Electroweak Stars powered by baryon number violating processes exist? • Can a star’s core be compressed to EW densities without being within its own RS? ...
Figure 3 - Scientific Research Publishing
Figure 3 - Scientific Research Publishing

... and quark-electron does not annihilate and what interactions cause them to unite in a completely stable particle - proton, which decays in nature is not observed. This consent of estimates and measured data indicates that the neutron is not an elementary particle. It should be seen as a some relativ ...
LA RIVELAZIONE DELLE PARTICELLE ELEMENTARI
LA RIVELAZIONE DELLE PARTICELLE ELEMENTARI

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Strangeness production



Strangeness production is a signature and a diagnostic tool of quark–gluon plasma (or QGP) formation and properties. Unlike up and down quarks, from which everyday matter is made, strange quarks are formed in pair-production processes in collisions between constituents of the plasma. The dominant mechanism of production involves gluons only present when matter has become a quark–gluon plasma. When quark–gluon plasma disassembles into hadrons in a breakup process, the high availability of strange antiquarks helps to produce antimatter containing multiple strange quarks, which is otherwise rarely made. Similar considerations are at present made for the heavier charm flavor, which is made at the beginning of the collision process in the first interactions and is only abundant in the high-energy environments of CERN's Large Hadron Collider.
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