78, 174508 (2008)
... the same temperature Tⴱ, where the pseudogap develops.2 Near optimum doping, the PKE appears at a temperature below Tc, which is consistent with the existence of a zerotemperature quantum phase transition under the superconducting dome. This observation suggests that the TR symmetry breaking and the ...
... the same temperature Tⴱ, where the pseudogap develops.2 Near optimum doping, the PKE appears at a temperature below Tc, which is consistent with the existence of a zerotemperature quantum phase transition under the superconducting dome. This observation suggests that the TR symmetry breaking and the ...
Taming instability of magnetic field in chiral medium
... to the chiral anomaly, the electromagnetic field and the medium exchange helicity which results in time-evolution of the chiral conductivity. Using the fastest growing momentum and helicity state of the vector potential as an ansatz, the time-evolution of the chiral conductivity and magnetic field i ...
... to the chiral anomaly, the electromagnetic field and the medium exchange helicity which results in time-evolution of the chiral conductivity. Using the fastest growing momentum and helicity state of the vector potential as an ansatz, the time-evolution of the chiral conductivity and magnetic field i ...
Towards Understanding the Internal Symmetries of Nature: Gauge
... However, we should all agree that there is at least one other class of phenomena operating in nature that are not distance-dependent. This class of real phenomena includes human consciousness, intention, emotion, mind, love, etc. This class of experimental data appears to require an “inward looking” ...
... However, we should all agree that there is at least one other class of phenomena operating in nature that are not distance-dependent. This class of real phenomena includes human consciousness, intention, emotion, mind, love, etc. This class of experimental data appears to require an “inward looking” ...
Introduction toElementary Particle Phenomenology
... so-called strange particles, relatively long-lived objects that were being produced in the new accelerator experiments. The long lifetimes of these particles suggested that, although the final states often only contained strongly interacting particles, they did not decay via the strong interaction; ...
... so-called strange particles, relatively long-lived objects that were being produced in the new accelerator experiments. The long lifetimes of these particles suggested that, although the final states often only contained strongly interacting particles, they did not decay via the strong interaction; ...
Proposal for a Detector of Photons with Zero Projection of... I. G. Savenko
... Here z is the direction of propagation and m∗ is the effective mass. A question arises: is it possible for a photon to have zero projection of spin and, even more significant, is it feasible to measure it or use? In this manuscript we propose an indirect method of detection of zero-spin photons and ...
... Here z is the direction of propagation and m∗ is the effective mass. A question arises: is it possible for a photon to have zero projection of spin and, even more significant, is it feasible to measure it or use? In this manuscript we propose an indirect method of detection of zero-spin photons and ...
Fulltext
... (4) scalar fields (which may account for the origin of masses). It is therefore natural to ask whether there exist stable stellar configurations other than dwarfs, neutron stars, and black holes. The central density of a typical neutron star is often greater than several times the nuclear matter den ...
... (4) scalar fields (which may account for the origin of masses). It is therefore natural to ask whether there exist stable stellar configurations other than dwarfs, neutron stars, and black holes. The central density of a typical neutron star is often greater than several times the nuclear matter den ...
Particle Physics in the LHC Era - SUrface
... gradually uncover new layers of physics, we can analyze them in an orderly fashion and then systematically incorporate them. Decoupling is the reason we do not need a detailed understanding of planetary geography and composition to understand how the sun and planets interact with one another. It is ...
... gradually uncover new layers of physics, we can analyze them in an orderly fashion and then systematically incorporate them. Decoupling is the reason we do not need a detailed understanding of planetary geography and composition to understand how the sun and planets interact with one another. It is ...
Supersymmetry and Gauge Theory (7CMMS41)
... theories are gauge theories. What does this mean? Well it is sometimes said that quantum field theories only make sense if they are renormalizable. Renormalizable means that all the divergences that arise in calculations can be compensated for by a (divergent) shift of the parameters of the theory ( ...
... theories are gauge theories. What does this mean? Well it is sometimes said that quantum field theories only make sense if they are renormalizable. Renormalizable means that all the divergences that arise in calculations can be compensated for by a (divergent) shift of the parameters of the theory ( ...
Magnetoexcitons break antiunitary symmetries
... results presented in Fig. 1 we used the constant value of B = 3 T and exciton states within a certain energy range. It is well known from atomic physics that chaotic effects become more apparent in higher magnetic fields or by using states of higher energies for the analysis. Hence, by increasing B ...
... results presented in Fig. 1 we used the constant value of B = 3 T and exciton states within a certain energy range. It is well known from atomic physics that chaotic effects become more apparent in higher magnetic fields or by using states of higher energies for the analysis. Hence, by increasing B ...
Chiral charge pumping in graphene deposited on a magnetic insulator
... errors. Thus, the existence of a circular induced electric field can be excluded. Figure 1(c) shows a typical dependence of the measured voltage versus the applied magnetic field. Comparing Figs. 1(b) and 1(c), one sees that the dc-voltage in SLG is induced at the same values of H 0 , where the effi ...
... errors. Thus, the existence of a circular induced electric field can be excluded. Figure 1(c) shows a typical dependence of the measured voltage versus the applied magnetic field. Comparing Figs. 1(b) and 1(c), one sees that the dc-voltage in SLG is induced at the same values of H 0 , where the effi ...
The Impossible Electric Dark Matter Black Hole
... Tandem Higgs). AS A RESULT, Free energy devices and electron-muon decay levitation is proposed. An unstable Higgs vacuum seems to be present around all black hole horizons by observed H2 production and annihilation radiation created by pair production of positrons and electrons. (Instability of the ...
... Tandem Higgs). AS A RESULT, Free energy devices and electron-muon decay levitation is proposed. An unstable Higgs vacuum seems to be present around all black hole horizons by observed H2 production and annihilation radiation created by pair production of positrons and electrons. (Instability of the ...
Atom Interferometry test of short range gravity : recent progress
... By properly modelling the Casimir Polder potential induced by the di-electric mirror on the atomic dipole. ...
... By properly modelling the Casimir Polder potential induced by the di-electric mirror on the atomic dipole. ...
Effect of the symmetry energy on gravitational waves from axial
... There are two classes of vector spherical harmonics (polar and axial) which are build out of combinations of the Levi-Civita volume form and the gradient operator acting on the scalar spherical harmonics. The difference between the two families is their parity. Under the parity operator π (under the ...
... There are two classes of vector spherical harmonics (polar and axial) which are build out of combinations of the Levi-Civita volume form and the gradient operator acting on the scalar spherical harmonics. The difference between the two families is their parity. Under the parity operator π (under the ...
Magnetoelectric coupling in the multiferroic compound LiCu O * Chen Fang,
... In this paper we introduce a theoretical model involving an interchain magnetoelectric coupling to provide an explanation for the experimental data on LiCu2O2.8–11 For LiCu2O2, there are two chains in each unit cell. Therefore, there are two types of “interchain” interactions. The first one is the i ...
... In this paper we introduce a theoretical model involving an interchain magnetoelectric coupling to provide an explanation for the experimental data on LiCu2O2.8–11 For LiCu2O2, there are two chains in each unit cell. Therefore, there are two types of “interchain” interactions. The first one is the i ...
berezinskii-kosterlitz-thouless transition and the haldane conjecture
... (with phases on both sides), and the model is considered uninteresting. However, the Ising model does have a finite This section deals with the 2D XY model, which is among the critical temperature in dimension d = 2 [6] or higher, and the classical spin models introduced in Section 1. We can imagine ...
... (with phases on both sides), and the model is considered uninteresting. However, the Ising model does have a finite This section deals with the 2D XY model, which is among the critical temperature in dimension d = 2 [6] or higher, and the classical spin models introduced in Section 1. We can imagine ...
In fla tio n
... exists, then nucleosynthesis would not work if BB started at kT > 109 GeV. Moduli: Spin-0 particles from superstring theory, contents of vacuum at high ...
... exists, then nucleosynthesis would not work if BB started at kT > 109 GeV. Moduli: Spin-0 particles from superstring theory, contents of vacuum at high ...
Oscillation Modes of Strange Quark Stars with a Strangelet Crust
... core, we adopt the Bag model EOS to describe the crust strangelets with O(m4s ) corrections, from which it follows that to the same order: nQ (µq ) = m2s µq /(2π 2 ) and χQ (µq ) = (2µ2q )/(π 2 ). Homogeneous quark matter gives way to the mixed phase crust at a radius r=rc where ξ|r=rc =1. The model ...
... core, we adopt the Bag model EOS to describe the crust strangelets with O(m4s ) corrections, from which it follows that to the same order: nQ (µq ) = m2s µq /(2π 2 ) and χQ (µq ) = (2µ2q )/(π 2 ). Homogeneous quark matter gives way to the mixed phase crust at a radius r=rc where ξ|r=rc =1. The model ...
The Origin of Matter-Antimatter Asymmetry Ning Bao Prashant Saraswat
... Since B – L conserved, a net lepton number can be converted into a baryon number through this process. Don’t need EWPT– since leptons are lighter than baryons, they go into equilibrium preferentially. Parameter space for this theory is accessible to current neutrino ...
... Since B – L conserved, a net lepton number can be converted into a baryon number through this process. Don’t need EWPT– since leptons are lighter than baryons, they go into equilibrium preferentially. Parameter space for this theory is accessible to current neutrino ...
G060296-00
... Spectra: provide a complete classification of non-linear harmonics, i.e. composition frequencies and sub-harmonics. Wave forms: determine more accurate templates for GW detection in the high frequency band. Nonlinear perturbation theory can be a complementary approach for investigating the above ...
... Spectra: provide a complete classification of non-linear harmonics, i.e. composition frequencies and sub-harmonics. Wave forms: determine more accurate templates for GW detection in the high frequency band. Nonlinear perturbation theory can be a complementary approach for investigating the above ...
Dark matter, neutron stars and strange quark matter
... ones have lifetimes of days. Since this time-scale is larger than the conversion time-scale tconv ≈ 100 s [21], it is in principle possible that strange stars could be formed if this conversion is triggered. As an estimate, the rate of formation of long-lived strangelets with, for example, A = 10 wo ...
... ones have lifetimes of days. Since this time-scale is larger than the conversion time-scale tconv ≈ 100 s [21], it is in principle possible that strange stars could be formed if this conversion is triggered. As an estimate, the rate of formation of long-lived strangelets with, for example, A = 10 wo ...
21_published article 4
... their impact on society is expected to be wide spread and all pervasive. By definition, a three dimensional object is chiral if it cannot be brought into congruence with its mirror image by any amount of translation and rotation. ...
... their impact on society is expected to be wide spread and all pervasive. By definition, a three dimensional object is chiral if it cannot be brought into congruence with its mirror image by any amount of translation and rotation. ...
PowerPoint 프레젠테이션
... Maximum NS mass can be any value within 1.5~1.8 Msun as far as supercritical accretion is concerned unseen “NS+LMBH” are 5 times more dominant than seen “NS+NS” system. “NS+LMBH” system may increase LIGO detection rate by factor of about 10. Possibilities of investigating NS inner structure vi ...
... Maximum NS mass can be any value within 1.5~1.8 Msun as far as supercritical accretion is concerned unseen “NS+LMBH” are 5 times more dominant than seen “NS+NS” system. “NS+LMBH” system may increase LIGO detection rate by factor of about 10. Possibilities of investigating NS inner structure vi ...
A New Constraint on Strongly Coupled Field Theories
... strongly coupled field theory, we are often guided by the idea that the number of massless particles is as small as possible. Since the anomaly condition can always be satisfied by a massless spectrum identical to the ultraviolet degrees of freedom, this would disfavor massless composites if the num ...
... strongly coupled field theory, we are often guided by the idea that the number of massless particles is as small as possible. Since the anomaly condition can always be satisfied by a massless spectrum identical to the ultraviolet degrees of freedom, this would disfavor massless composites if the num ...
New Scientist - Quark Nova Project
... with a crust of iron. Whirling up to 1000 times per second, a neutron star is constantly shedding magnetic fields. Over time, this loss of energy causes the star to spin slower and slower. As it spins down, the centrifugal forces that kept gravity at bay start weakening, allowing gravity to squish t ...
... with a crust of iron. Whirling up to 1000 times per second, a neutron star is constantly shedding magnetic fields. Over time, this loss of energy causes the star to spin slower and slower. As it spins down, the centrifugal forces that kept gravity at bay start weakening, allowing gravity to squish t ...
