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		<title>Turkey earthquake reveals a new active fault zone</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/wDbiuhZwQJA/</link>
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		<pubDate>Mon, 24 Oct 2011 14:08:40 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[Physics News]]></category>
		<category><![CDATA[Active]]></category>
		<category><![CDATA[Earthquake]]></category>
		<category><![CDATA[fault]]></category>
		<category><![CDATA[reveals]]></category>
		<category><![CDATA[Turkey]]></category>
		<category><![CDATA[zone]]></category>

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		<description><![CDATA[<p>Recent earthquakes in Turkey have occurred along one or other of the country&#8217;s two main faults. Yesterday&#8217;s quake struck near their meeting point<img width='1' height='1' src='http://feeds.newscientist.com/c/749/f/424049/s/1983d863/mf.gif' border='0'/>
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<a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://feeds.newscientist.com/c/749/f/424049/s/1983d863/l/0L0Snewscientist0N0Carticle0Cdn210A830Eturkey0Eearthquake0Ereveals0Ea0Enew0Eactive0Efault0Ezone0Bhtml0DDCMP0FOTC0Erss0Gnsref0Fphysics0Emath/story01.htm" rel="nofollow" >New Scientist &#8211; Physics &#038; Math</a>&#8230; <a href="http://www.actaphysica.com/physics-news/turkey-earthquake-reveals-a-new-active-fault-zone/" class="read_more">Continue reading ...</a></p>]]></description>
			<content:encoded><![CDATA[<p>Recent earthquakes in Turkey have occurred along one or other of the country&#8217;s two main faults. Yesterday&#8217;s quake struck near their meeting point<img width='1' height='1' src='http://feeds.newscientist.com/c/749/f/424049/s/1983d863/mf.gif' border='0'/>
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		<title>Shear modulus of the hadron-quark mixed phase. (arXiv:1110.4650v1 [astro-ph.SR])</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/mKZzWrH3IPE/</link>
		<comments>http://www.actaphysica.com/latest-physics-research/high-energy-physics/shear-modulus-of-the-hadron-quark-mixed-phase-arxiv1110-4650v1-astro-ph-sr/#comments</comments>
		<pubDate>Mon, 24 Oct 2011 12:59:43 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[High-Energy Physics]]></category>
		<category><![CDATA[arXiv1110.4650v1]]></category>
		<category><![CDATA[astroph.SR]]></category>
		<category><![CDATA[hadronquark]]></category>
		<category><![CDATA[Mixed]]></category>
		<category><![CDATA[modulus]]></category>
		<category><![CDATA[phase]]></category>
		<category><![CDATA[Shear]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/latest-physics-research/high-energy-physics/shear-modulus-of-the-hadron-quark-mixed-phase-arxiv1110-4650v1-astro-ph-sr/</guid>
		<description><![CDATA[<p>Robust arguments predict that a hadron-quark mixed phase may exist in the<br />
cores of some &#8220;neutron&#8221; stars. Such a phase forms a crystalline lattice with a<br />
shear modulus higher than that of the crust due to the high density and charge<br />
separation, even allowing for the effects of charge screening. This may lead to<br />
strong continuous gravitational-wave emission from rapidly rotating neutron<br />
stars and gravitational-wave bursts associated with magnetar flares and pulsar<br />
glitches. We present the first detailed calculation of the shear modulus of the<br />
mixed phase. We describe the quark phase using the bag model plus first-order<br />
quantum chromodynamics corrections and the hadronic phase using relativistic<br />
mean-field models with parameters allowed by the most massive pulsar. Most of<br />
the calculation involves treating the &#8220;pasta phases&#8221; of the lattice via<br />
dimensional continuation, and we give a general method for computing<br />
dimensionally continued lattice sums including the Debye model of charge<br />
screening. We compute all the shear components of the elastic modulus tensor<br />
and angle average them to obtain the effective (scalar) shear modulus for the<br />
case where the mixed phase is a polycrystal. We include the contributions from<br />
changing the cell size, which are necessary for the stability of the<br />
lower-dimensional portions of the lattice. Stability also requires a minimum<br />
surface tension, generally tens of MeV/fm^2 depending on the equation of state.<br />
We find that the shear modulus can be a few times 10^33 erg/cm^3, two orders of<br />
magnitude higher than the first estimate, over a significant fraction of the<br />
maximum mass stable star for certain parameter choices.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4650" rel="nofollow" >hep-ph updates on arXiv.org</a>&#8230; <a href="http://www.actaphysica.com/latest-physics-research/high-energy-physics/shear-modulus-of-the-hadron-quark-mixed-phase-arxiv1110-4650v1-astro-ph-sr/" class="read_more">Continue reading ...</a></p>]]></description>
			<content:encoded><![CDATA[<p>Robust arguments predict that a hadron-quark mixed phase may exist in the<br />
cores of some &#8220;neutron&#8221; stars. Such a phase forms a crystalline lattice with a<br />
shear modulus higher than that of the crust due to the high density and charge<br />
separation, even allowing for the effects of charge screening. This may lead to<br />
strong continuous gravitational-wave emission from rapidly rotating neutron<br />
stars and gravitational-wave bursts associated with magnetar flares and pulsar<br />
glitches. We present the first detailed calculation of the shear modulus of the<br />
mixed phase. We describe the quark phase using the bag model plus first-order<br />
quantum chromodynamics corrections and the hadronic phase using relativistic<br />
mean-field models with parameters allowed by the most massive pulsar. Most of<br />
the calculation involves treating the &#8220;pasta phases&#8221; of the lattice via<br />
dimensional continuation, and we give a general method for computing<br />
dimensionally continued lattice sums including the Debye model of charge<br />
screening. We compute all the shear components of the elastic modulus tensor<br />
and angle average them to obtain the effective (scalar) shear modulus for the<br />
case where the mixed phase is a polycrystal. We include the contributions from<br />
changing the cell size, which are necessary for the stability of the<br />
lower-dimensional portions of the lattice. Stability also requires a minimum<br />
surface tension, generally tens of MeV/fm^2 depending on the equation of state.<br />
We find that the shear modulus can be a few times 10^33 erg/cm^3, two orders of<br />
magnitude higher than the first estimate, over a significant fraction of the<br />
maximum mass stable star for certain parameter choices.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4650" rel="nofollow" >hep-ph updates on arXiv.org</a></p>

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		<title>Origin and meaning of quantum nonlocality. (arXiv:1110.4641v1 [quant-ph])</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/ptgHKyJhUJc/</link>
		<comments>http://www.actaphysica.com/latest-physics-research/quantum-physics/origin-and-meaning-of-quantum-nonlocality-arxiv1110-4641v1-quant-ph/#comments</comments>
		<pubDate>Mon, 24 Oct 2011 11:06:44 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[Quantum Physics]]></category>
		<category><![CDATA[arXiv1110.4641v1]]></category>
		<category><![CDATA[meaning]]></category>
		<category><![CDATA[Nonlocality]]></category>
		<category><![CDATA[Origin]]></category>
		<category><![CDATA[quantph]]></category>
		<category><![CDATA[Quantum]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/latest-physics-research/quantum-physics/origin-and-meaning-of-quantum-nonlocality-arxiv1110-4641v1-quant-ph/</guid>
		<description><![CDATA[<p>Quantum nonlocality is revisited from a novel point of view by studying the<br />
problem of an originally classical particle immersed in the stochastic<br />
zero-point radiation field (zpf). The entire system is left to evolve until it<br />
reaches a state in which the radiative terms cancel each other in the mean in a<br />
first approximation. The ensuing approximate statistical description reduced to<br />
the particle&#8217;s configuration space contains a nonclassical term due to the<br />
dispersion of the momentum, which depends on the density of particles {\rho}(x)<br />
and thus is nonlocal. This description is shown to be equivalent to<br />
Schr\&#8221;odinger&#8217;s equation and its complex conjugate. The nonlocal term is<br />
recognized as the so-called quantum potential, thus solving the long standing<br />
problem of the origin and meaning of this term. Further, the relationship<br />
between the Wigner function and a true Kolmogorovian probability density in<br />
phase space is discussed from the perspective provided by this theory.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4641" rel="nofollow" >quant-ph updates on arXiv.org</a></p>
<h4>Incoming search terms:</h4><ul><li><a href="http://www.actaphysica.com/latest-physics-research/quantum-physics/origin-and-meaning-of-quantum-nonlocality-arxiv1110-4641v1-quant-ph/"  title="arxiv quantum non-locality">arxiv quantum non-locality</a></li>&#8230; <a href="http://www.actaphysica.com/latest-physics-research/quantum-physics/origin-and-meaning-of-quantum-nonlocality-arxiv1110-4641v1-quant-ph/" class="read_more">Continue reading ...</a></ul>]]></description>
			<content:encoded><![CDATA[<p>Quantum nonlocality is revisited from a novel point of view by studying the<br />
problem of an originally classical particle immersed in the stochastic<br />
zero-point radiation field (zpf). The entire system is left to evolve until it<br />
reaches a state in which the radiative terms cancel each other in the mean in a<br />
first approximation. The ensuing approximate statistical description reduced to<br />
the particle&#8217;s configuration space contains a nonclassical term due to the<br />
dispersion of the momentum, which depends on the density of particles {\rho}(x)<br />
and thus is nonlocal. This description is shown to be equivalent to<br />
Schr\&#8221;odinger&#8217;s equation and its complex conjugate. The nonlocal term is<br />
recognized as the so-called quantum potential, thus solving the long standing<br />
problem of the origin and meaning of this term. Further, the relationship<br />
between the Wigner function and a true Kolmogorovian probability density in<br />
phase space is discussed from the perspective provided by this theory.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4641" rel="nofollow" >quant-ph updates on arXiv.org</a></p>
<h4>Incoming search terms:</h4><ul><li><a href="http://www.actaphysica.com/latest-physics-research/quantum-physics/origin-and-meaning-of-quantum-nonlocality-arxiv1110-4641v1-quant-ph/"  title="arxiv quantum non-locality">arxiv quantum non-locality</a></li></ul>
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		<title>SLAC software developer discusses physics simulation tool to make cancer therapy safer</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/DW4iscbvN-c/</link>
		<comments>http://www.actaphysica.com/physics-news/slac-software-developer-discusses-physics-simulation-tool-to-make-cancer-therapy-safer/#comments</comments>
		<pubDate>Mon, 24 Oct 2011 07:10:03 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[Physics News]]></category>
		<category><![CDATA[cancer]]></category>
		<category><![CDATA[developer]]></category>
		<category><![CDATA[Discusses]]></category>
		<category><![CDATA[physics]]></category>
		<category><![CDATA[safer]]></category>
		<category><![CDATA[Simulation]]></category>
		<category><![CDATA[SLAC]]></category>
		<category><![CDATA[Software]]></category>
		<category><![CDATA[therapy]]></category>
		<category><![CDATA[Tool]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/physics-news/slac-software-developer-discusses-physics-simulation-tool-to-make-cancer-therapy-safer/</guid>
		<description><![CDATA[<p>Tiny particles are making a big difference in the world of cancer therapy. And SLAC physicists&#8212;experts in particle transport&#8212;are using computer simulations to make those therapies safer.<br />
<a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://www.physorg.com/news/2011-10-slac-software-discusses-physics-simulation.html" rel="nofollow" >PHYSorg.com: Physics News</a>&#8230; <a href="http://www.actaphysica.com/physics-news/slac-software-developer-discusses-physics-simulation-tool-to-make-cancer-therapy-safer/" class="read_more">Continue reading ...</a></p>]]></description>
			<content:encoded><![CDATA[<p>Tiny particles are making a big difference in the world of cancer therapy. And SLAC physicists&#8212;experts in particle transport&#8212;are using computer simulations to make those therapies safer.<br />
<a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://www.physorg.com/news/2011-10-slac-software-discusses-physics-simulation.html" rel="nofollow" >PHYSorg.com: Physics News</a></p>

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		<title>Quantum Mechanics, Spacetime Locality, and Gravity. (arXiv:1110.4630v1 [hep-th])</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/Ng8L6BFG0MU/</link>
		<comments>http://www.actaphysica.com/latest-physics-research/high-energy-physics/quantum-mechanics-spacetime-locality-and-gravity-arxiv1110-4630v1-hep-th/#comments</comments>
		<pubDate>Mon, 24 Oct 2011 02:06:34 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[High-Energy Physics]]></category>
		<category><![CDATA[arXiv1110.4630v1]]></category>
		<category><![CDATA[Gravity]]></category>
		<category><![CDATA[hepth]]></category>
		<category><![CDATA[locality]]></category>
		<category><![CDATA[Mechanics]]></category>
		<category><![CDATA[Quantum]]></category>
		<category><![CDATA[Spacetime.]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/latest-physics-research/high-energy-physics/quantum-mechanics-spacetime-locality-and-gravity-arxiv1110-4630v1-hep-th/</guid>
		<description><![CDATA[<p>Quantum mechanics introduces the concept of probability at the fundamental<br />
level, yielding the measurement problem. On the other hand, recent progress in<br />
cosmology has led to the &#8220;multiverse&#8221; picture, in which our observed universe<br />
is only one of the many, bringing an apparent arbitrariness in defining<br />
probabilities, called the measure problem.
</p>
<p>In this paper, we discuss how these two problems are intimately related with<br />
each other, developing a complete picture for quantum measurement and<br />
cosmological histories in the quantum mechanical universe. On one hand, quantum<br />
mechanics eliminates the arbitrariness of defining probabilities in the<br />
multiverse, as discussed in <a href="/abs/1104.2324">arXiv:1104.2324</a>. On the other hand, the multiverse<br />
allows for understanding why we observe an ordered world obeying consistent<br />
laws of physics, by providing an infinite-dimensional Hilbert space. This<br />
results in the irreversibility of quantum measurement, despite the fact that<br />
the evolution of the multiverse state is unitary.
</p>
<p>In order to describe the cosmological dynamics correctly, we need to identify<br />
the structure of the Hilbert space for a system with gravity. We argue that in<br />
order to keep spacetime locality, the Hilbert space for dynamical spacetime<br />
must be defined only in restricted spacetime regions: in and on the (stretched)<br />
apparent horizon as viewed from a fixed reference frame. This requirement<br />
arises from eliminating all the redundancies and overcountings in a general<br />
relativistic, global spacetime description of nature. It is responsible for<br />
horizon complementarity as well as the &#8220;observer dependence&#8221; of<br />
horizons/spacetime&#8212;these phenomena arise to represent changes of the<br />
reference frame in the relevant Hilbert space. This can be viewed as an<br />
extension of the Poincare transformation in the quantum gravitational context,<br />
as the Lorentz transformation is viewed as an extension of the Galilean<br />
transformation.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4630" rel="nofollow" >hep-th updates on arXiv.org</a>&#8230; <a href="http://www.actaphysica.com/latest-physics-research/high-energy-physics/quantum-mechanics-spacetime-locality-and-gravity-arxiv1110-4630v1-hep-th/" class="read_more">Continue reading ...</a></p>]]></description>
			<content:encoded><![CDATA[<p>Quantum mechanics introduces the concept of probability at the fundamental<br />
level, yielding the measurement problem. On the other hand, recent progress in<br />
cosmology has led to the &#8220;multiverse&#8221; picture, in which our observed universe<br />
is only one of the many, bringing an apparent arbitrariness in defining<br />
probabilities, called the measure problem.
</p>
<p>In this paper, we discuss how these two problems are intimately related with<br />
each other, developing a complete picture for quantum measurement and<br />
cosmological histories in the quantum mechanical universe. On one hand, quantum<br />
mechanics eliminates the arbitrariness of defining probabilities in the<br />
multiverse, as discussed in <a href="/abs/1104.2324">arXiv:1104.2324</a>. On the other hand, the multiverse<br />
allows for understanding why we observe an ordered world obeying consistent<br />
laws of physics, by providing an infinite-dimensional Hilbert space. This<br />
results in the irreversibility of quantum measurement, despite the fact that<br />
the evolution of the multiverse state is unitary.
</p>
<p>In order to describe the cosmological dynamics correctly, we need to identify<br />
the structure of the Hilbert space for a system with gravity. We argue that in<br />
order to keep spacetime locality, the Hilbert space for dynamical spacetime<br />
must be defined only in restricted spacetime regions: in and on the (stretched)<br />
apparent horizon as viewed from a fixed reference frame. This requirement<br />
arises from eliminating all the redundancies and overcountings in a general<br />
relativistic, global spacetime description of nature. It is responsible for<br />
horizon complementarity as well as the &#8220;observer dependence&#8221; of<br />
horizons/spacetime&#8212;these phenomena arise to represent changes of the<br />
reference frame in the relevant Hilbert space. This can be viewed as an<br />
extension of the Poincare transformation in the quantum gravitational context,<br />
as the Lorentz transformation is viewed as an extension of the Galilean<br />
transformation.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4630" rel="nofollow" >hep-th updates on arXiv.org</a></p>

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		<item>
		<title>Vote Now! Top Space Stories of the Week – Oct. 23, 2011</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/xqNbdlCK09w/</link>
		<comments>http://www.actaphysica.com/physics-news/vote-now-top-space-stories-of-the-week-oct-23-2011/#comments</comments>
		<pubDate>Mon, 24 Oct 2011 00:08:53 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[Physics News]]></category>
		<category><![CDATA[2011]]></category>
		<category><![CDATA[Oct.]]></category>
		<category><![CDATA[Space]]></category>
		<category><![CDATA[Stories]]></category>
		<category><![CDATA[Vote]]></category>
		<category><![CDATA[Week]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/physics-news/vote-now-top-space-stories-of-the-week-oct-23-2011/</guid>
		<description><![CDATA[<p>Was it the doomed falling satellite, the possibilities of vacations to space or something else?</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://feedads.g.doubleclick.net/~a/J8NgxR9RReS3Oum3FGvVotNLNHg/0/da" ><img src="http://feedads.g.doubleclick.net/~a/J8NgxR9RReS3Oum3FGvVotNLNHg/0/di" border="0" ismap="true"/></a><br />
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<p><img src="http://feeds.feedburner.com/~r/spaceheadlines/~4/nTnacEIl3yU" height="1" width="1"/><br />
<a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://feedproxy.google.com/~r/spaceheadlines/~3/nTnacEIl3yU/13361-vote-top-space-stories-week-october-23-2011.html" rel="nofollow" >SPACE.com</a>&#8230; <a href="http://www.actaphysica.com/physics-news/vote-now-top-space-stories-of-the-week-oct-23-2011/" class="read_more">Continue reading ...</a></p>]]></description>
			<content:encoded><![CDATA[<p>Was it the doomed falling satellite, the possibilities of vacations to space or something else?</p>
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		<item>
		<title>The Dark Matter &amp; Dark Energy [1/5]</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/_DOKL9BVjg0/</link>
		<comments>http://www.actaphysica.com/physics-videos/the-dark-matter-dark-energy-15-2/#comments</comments>
		<pubDate>Sun, 23 Oct 2011 17:15:58 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[Physics Videos]]></category>
		<category><![CDATA[Dark]]></category>
		<category><![CDATA[Energy]]></category>
		<category><![CDATA[Matter]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/physics-videos/the-dark-matter-dark-energy-15-2/</guid>
		<description><![CDATA[<p>				
				</p>
<p>Dark matter are invisible objects that react with matter by gravitational force. Scientists believe that the dark matter is made up of exotic particles like WIMPs(Weakly Interacting Massive Particles).In physical cosmology, dark energy is an exotic form of energy that permeates all of space and tends to increase the rate of expansion of the universe.Dark energy is the most popular way to explain recent observations that the universe appears to be expanding at an accelerating rate. In the standard model of cosmology, dark energy currently accounts for 73% of the total mass-energy of the universe.
</p>
<p>				
				</p>
<p>History Channel The Universe Dark Matter</p>
<h4>Incoming search terms:</h4><ul><li><a href="http://www.actaphysica.com/physics-videos/the-dark-matter-dark-energy-15-2/"  title="the dark matter &#38; dark energy [1/5]">the dark matter &#38; dark energy [1/5]</a></li>&#8230; <a href="http://www.actaphysica.com/physics-videos/the-dark-matter-dark-energy-15-2/" class="read_more">Continue reading ...</a></ul>]]></description>
			<content:encoded><![CDATA[<p>				<object width="425" height="355"><param name="movie" value="http://www.youtube.com/v/rLmcbjLVPKc?fs=1"></param><param name="allowFullScreen" value="true"></param>
				<embed src="http://www.youtube.com/v/rLmcbjLVPKc?fs=1&#038;rel=0" type="application/x-shockwave-flash" width="425" height="355" allowfullscreen="true"></embed></object></p>
<p>Dark matter are invisible objects that react with matter by gravitational force. Scientists believe that the dark matter is made up of exotic particles like WIMPs(Weakly Interacting Massive Particles).In physical cosmology, dark energy is an exotic form of energy that permeates all of space and tends to increase the rate of expansion of the universe.Dark energy is the most popular way to explain recent observations that the universe appears to be expanding at an accelerating rate. In the standard model of cosmology, dark energy currently accounts for 73% of the total mass-energy of the universe.
</p>
<p>				<object width="425" height="355"><param name="movie" value="http://www.youtube.com/v/cd7XCC42ayw?fs=1"></param><param name="allowFullScreen" value="true"></param>
				<embed src="http://www.youtube.com/v/cd7XCC42ayw?fs=1&#038;rel=0" type="application/x-shockwave-flash" width="425" height="355" allowfullscreen="true"></embed></object></p>
<p>History Channel The Universe Dark Matter</p>
<h4>Incoming search terms:</h4><ul><li><a href="http://www.actaphysica.com/physics-videos/the-dark-matter-dark-energy-15-2/"  title="the dark matter &amp; dark energy [1/5]">the dark matter &amp; dark energy [1/5]</a></li></ul>
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		<title>Vehicle Preps, Inspections, Plumbing and Science for Station Crew</title>
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		<comments>http://www.actaphysica.com/physics-news/vehicle-preps-inspections-plumbing-and-science-for-station-crew/#comments</comments>
		<pubDate>Sun, 23 Oct 2011 17:09:10 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[Physics News]]></category>
		<category><![CDATA[Crew]]></category>
		<category><![CDATA[Inspections]]></category>
		<category><![CDATA[Plumbing]]></category>
		<category><![CDATA[Preps]]></category>
		<category><![CDATA[Science]]></category>
		<category><![CDATA[Station]]></category>
		<category><![CDATA[Vehicle]]></category>

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		<description><![CDATA[<p>The Expedition 29 crew wrapped up its work week conducting inspection and plumbing work. They performed ongoing science and readied a supply ship for undocking. Meanwhile in Russia, the ISS Progress 45 resupply craft is being prepared for launch with docking planned for Nov. 2. </p>
<p>Commander Mike Fossum spent time on the Binary Colloidal Alloy Test experiment which observes microscopic particles, or colloids, suspended in a liquid. He photographed samples from the experiment that could lead to i&#160;[...]</p>
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			<content:encoded><![CDATA[<p>The Expedition 29 crew wrapped up its work week conducting inspection and plumbing work. They performed ongoing science and readied a supply ship for undocking. Meanwhile in Russia, the ISS Progress 45 resupply craft is being prepared for launch with docking planned for Nov. 2. </p>
<p>Commander Mike Fossum spent time on the Binary Colloidal Alloy Test experiment which observes microscopic particles, or colloids, suspended in a liquid. He photographed samples from the experiment that could lead to i&nbsp;[...]</p>
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		<title>Dark Matter after BESS-Polar II. (arXiv:1110.4376v1 [hep-ph])</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/-r9pxNYLQ-c/</link>
		<comments>http://www.actaphysica.com/latest-physics-research/high-energy-physics/dark-matter-after-bess-polar-ii-arxiv1110-4376v1-hep-ph/#comments</comments>
		<pubDate>Sun, 23 Oct 2011 17:06:31 +0000</pubDate>
		<dc:creator />
				<category><![CDATA[High-Energy Physics]]></category>
		<category><![CDATA[after]]></category>
		<category><![CDATA[arXiv1110.4376v1]]></category>
		<category><![CDATA[BESSPolar]]></category>
		<category><![CDATA[Dark]]></category>
		<category><![CDATA[hepph]]></category>
		<category><![CDATA[Matter]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/latest-physics-research/high-energy-physics/dark-matter-after-bess-polar-ii-arxiv1110-4376v1-hep-ph/</guid>
		<description><![CDATA[<p>The BESS-Polar collaboration has recently performed a precise measurement of<br />
the local antiproton flux which is consistent with a pure secondary production<br />
of antiprotons. We constrain a possible primary component originating from dark<br />
matter pair-annihilations. We derive limits on the annihilation cross section<br />
which are stronger than or comparable to those from the PAMELA satellite<br />
experiment for dark matter masses up to 200 GeV. Especially, we exclude thermal<br />
WIMPs with masses in the range 3-20 GeV if they annihilate dominantly into<br />
quark pairs unless their cross section is velocity suppressed.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4376" rel="nofollow" >hep-ph updates on arXiv.org</a>&#8230; <a href="http://www.actaphysica.com/latest-physics-research/high-energy-physics/dark-matter-after-bess-polar-ii-arxiv1110-4376v1-hep-ph/" class="read_more">Continue reading ...</a></p>]]></description>
			<content:encoded><![CDATA[<p>The BESS-Polar collaboration has recently performed a precise measurement of<br />
the local antiproton flux which is consistent with a pure secondary production<br />
of antiprotons. We constrain a possible primary component originating from dark<br />
matter pair-annihilations. We derive limits on the annihilation cross section<br />
which are stronger than or comparable to those from the PAMELA satellite<br />
experiment for dark matter masses up to 200 GeV. Especially, we exclude thermal<br />
WIMPs with masses in the range 3-20 GeV if they annihilate dominantly into<br />
quark pairs unless their cross section is velocity suppressed.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4376" rel="nofollow" >hep-ph updates on arXiv.org</a></p>

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		<title>Heavy Quark Dynamics in the QGP. (arXiv:1110.4138v1 [hep-ph])</title>
		<link>http://feedproxy.google.com/~r/Actaphysica/~3/8sDJgQs4fBQ/</link>
		<comments>http://www.actaphysica.com/latest-physics-research/high-energy-physics/heavy-quark-dynamics-in-the-qgp-arxiv1110-4138v1-hep-ph/#comments</comments>
		<pubDate>Thu, 20 Oct 2011 09:14:36 +0000</pubDate>
		<dc:creator>Actaphysica</dc:creator>
				<category><![CDATA[High-Energy Physics]]></category>
		<category><![CDATA[arXiv1110.4138v1]]></category>
		<category><![CDATA[Dynamics.]]></category>
		<category><![CDATA[heavy]]></category>
		<category><![CDATA[hepph]]></category>
		<category><![CDATA[QGP.]]></category>
		<category><![CDATA[quark]]></category>

		<guid isPermaLink="false">http://www.actaphysica.com/latest-physics-research/high-energy-physics/heavy-quark-dynamics-in-the-qgp-arxiv1110-4138v1-hep-ph/</guid>
		<description><![CDATA[<p>We assess transport properties of heavy quarks in the Quark-Gluon Plasma<br />
(QGP) that show a strong non-perturbative behavior. A T-matrix approach based<br />
on a potential taken from lattice QCD hints at the presence of heavy-quark (HQ)<br />
resonant scattering with an increasing strength as the temperature, $  T$  ,<br />
reaches the critical temperature, $  T_c \simeq 170 \; \MeV$   for deconfinement<br />
from above. The implementation of HQ resonance scattering along with a<br />
hadronization via quark coalescence under the conditions of the plasma created<br />
in heavy-ion collisions has been shown to correctly describe both the nuclear<br />
modification factor, $  R_{AA}$  , and the elliptic flow, $  v_2$  , of single<br />
electrons at RHIC and have correctly predicted the $  R_{AA}$   of D mesons at LHC<br />
energy.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4138" target="_blank" rel="nofollow" >hep-ph updates on arXiv.org</a>&#8230; <a href="http://www.actaphysica.com/latest-physics-research/high-energy-physics/heavy-quark-dynamics-in-the-qgp-arxiv1110-4138v1-hep-ph/" class="read_more">Continue reading ...</a></p>]]></description>
			<content:encoded><![CDATA[<p>We assess transport properties of heavy quarks in the Quark-Gluon Plasma<br />
(QGP) that show a strong non-perturbative behavior. A T-matrix approach based<br />
on a potential taken from lattice QCD hints at the presence of heavy-quark (HQ)<br />
resonant scattering with an increasing strength as the temperature, $  T$  ,<br />
reaches the critical temperature, $  T_c \simeq 170 \; \MeV$   for deconfinement<br />
from above. The implementation of HQ resonance scattering along with a<br />
hadronization via quark coalescence under the conditions of the plasma created<br />
in heavy-ion collisions has been shown to correctly describe both the nuclear<br />
modification factor, $  R_{AA}$  , and the elliptic flow, $  v_2$  , of single<br />
electrons at RHIC and have correctly predicted the $  R_{AA}$   of D mesons at LHC<br />
energy.
</p>
<p><a target="_blank" rel="nofollow" href="http://www.actaphysica.com/goto/http://arxiv.org/abs/1110.4138" target="_blank" rel="nofollow" >hep-ph updates on arXiv.org</a></p>

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