The Minimal CFL-Nuclear Interface
... Throughout the remainder of the paper, we will adopt the minimal hypothesis that nuclear matter composed of neutrons, protons and electrons, known to exist at densities of order n0 , and CFL matter, known to exist at asymptotically large densities, exhaust the content of a neutron star. We conclude ...
... Throughout the remainder of the paper, we will adopt the minimal hypothesis that nuclear matter composed of neutrons, protons and electrons, known to exist at densities of order n0 , and CFL matter, known to exist at asymptotically large densities, exhaust the content of a neutron star. We conclude ...
Matching next-to-leading order predictions to parton showers
... to resummed total rates combined with the next-to-leading order (NLO) result [9–13]. More sophisticated differential theoretical predictions are however always helpful for setting more accurate exclusion limits, possibly refining the search strategies, and measuring the model free parameters in case ...
... to resummed total rates combined with the next-to-leading order (NLO) result [9–13]. More sophisticated differential theoretical predictions are however always helpful for setting more accurate exclusion limits, possibly refining the search strategies, and measuring the model free parameters in case ...
Full-Wave Simulation of High-Frequency Electromagnetic
... explicitly 3D interaction, and its effects have been calculated. The broadening and defocusing effect on microwave beams caused by realistic edge turbulence, observed in all magnetic fusion devices, is also investigated. A fluid model for edge turbulence is used to produce realistic turbulent profil ...
... explicitly 3D interaction, and its effects have been calculated. The broadening and defocusing effect on microwave beams caused by realistic edge turbulence, observed in all magnetic fusion devices, is also investigated. A fluid model for edge turbulence is used to produce realistic turbulent profil ...
Advanced Concepts of Electromagnetic Generation, Confinement
... is orders of magnitude lower than for chemical thrusters, the continuous acceleration gained by a spacecraft propelled by such engines allows accomplishing very ambitious missions, whilst requiring relatively higher transfer times. On the other hand these engines demand for less propellant mass, tha ...
... is orders of magnitude lower than for chemical thrusters, the continuous acceleration gained by a spacecraft propelled by such engines allows accomplishing very ambitious missions, whilst requiring relatively higher transfer times. On the other hand these engines demand for less propellant mass, tha ...
HiggsIdentity_Part1
... the Higgs boson as well as the naturalness of the mass. • Composite Higgs models generally have a reduced gluon fusion rate. • Unnatural models tend to have an enhanced production rate. ...
... the Higgs boson as well as the naturalness of the mass. • Composite Higgs models generally have a reduced gluon fusion rate. • Unnatural models tend to have an enhanced production rate. ...
Charge dependent azimuthal correlations with the ALICE detector at
... Disadvantage: contamination from secondaries Investigated by varying the cut on the distance of closest approach (results used for the systematic uncertainty). ...
... Disadvantage: contamination from secondaries Investigated by varying the cut on the distance of closest approach (results used for the systematic uncertainty). ...
Strong Electroweak Symmetry Breaking
... answers exist but none has been shown to be true in experiment. One possibility in the Standard Model is that particles obtain mass through spontaneous symmetry breaking at the scale of the electroweak force. Spontaneous symmetry breaking can be understood with a “Mexican hat” depicting a potential ...
... answers exist but none has been shown to be true in experiment. One possibility in the Standard Model is that particles obtain mass through spontaneous symmetry breaking at the scale of the electroweak force. Spontaneous symmetry breaking can be understood with a “Mexican hat” depicting a potential ...
Effective Field Theory
... basic constituents of nature, which would unify the different kinds of interactions: the so-called theory of everything. However, even if such a marvelous theory is found at some point, a quantitative analysis at the most elementary level is going to be of little use for providing a comprehensive de ...
... basic constituents of nature, which would unify the different kinds of interactions: the so-called theory of everything. However, even if such a marvelous theory is found at some point, a quantitative analysis at the most elementary level is going to be of little use for providing a comprehensive de ...
1 - Indico
... Software to get the branching fractions right will be available before the LHC turns on ...
... Software to get the branching fractions right will be available before the LHC turns on ...
of satellite data, and associated opportunities for the LHC
... Recently reported possible satellite signals and relevant data: PAMELA, Fermi/GLAST, etc Dark matter! Not only learn what DM is – could also be the discovery of supersymmetry (if indeed LSP) – may also point toward underlying theory – probes cosmological history of universe! -Worth lot of effort to ...
... Recently reported possible satellite signals and relevant data: PAMELA, Fermi/GLAST, etc Dark matter! Not only learn what DM is – could also be the discovery of supersymmetry (if indeed LSP) – may also point toward underlying theory – probes cosmological history of universe! -Worth lot of effort to ...
What is the Higgs Boson?
... Schwinger (1957): a coupling produces effective mass terms through the action of the vacuum fluctuations (Higgs boson) Top quark most affected by this “Higgs field molasses” Note: Higgs couplings explain fundamental ...
... Schwinger (1957): a coupling produces effective mass terms through the action of the vacuum fluctuations (Higgs boson) Top quark most affected by this “Higgs field molasses” Note: Higgs couplings explain fundamental ...
dark matter effective field theories in stars
... dark matter abundance is defined by the time of WIMP freezeout, which happens when the universe’s temperature drops below the WIMPs mass, resulting in the decoupling of dark matter particles from the primordial universe thermal bath. This will result in a constant number of WIMPs per co-moving volume ...
... dark matter abundance is defined by the time of WIMP freezeout, which happens when the universe’s temperature drops below the WIMPs mass, resulting in the decoupling of dark matter particles from the primordial universe thermal bath. This will result in a constant number of WIMPs per co-moving volume ...
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.