Screening of Very Intense Magnetic Fields by Chiral Symmetry Breaking

In very intense magnetic fields, $B > 1.5\times 10^{14}$ T, the breaking of the strong interaction $SU(2)\times SU(2)$ symmetry arranges itself so that instead of the neutral $\sigma$ field acquiring a vacuum expectation value it is the charged $\pi$ field that does and the magnetic field is screened. Details are presented for a magnetic field generated by a current in a wire; we show that the magnetic field is screened out to a distance $\rho_o\sim I/f_\pi m_\pi$ from the wire.Comment: 7 pages (using macropackage REVTEX II

Hadronic Instabilities in Very Intense Magnetic Fields

Composite hadronic states exhibit interesting properties in the presence of very intense magnetic fields, such as those conjectured to exist in the vicinity of certain astrophysical objects. We discuss three scenarios. (i) The presence of vector particles with anomalous magnetic moment couplings to scalar particles, induces an instability of the vacuum. (ii) A delicate interplay between the anomalous magnetic moments of the proton and neutron makes, in magnetic fields $B\ge 2\times 10^{14}$ T, the neutron stable and for fields $B\ge 5\times 10^{14}$ T the proton becomes unstable to a decay into a neutron via $\beta$ emission. (iii) In the unbroken chiral $\sigma$ model magnetic fields would be screened out as in a superconductor. It is the explicit breaking of chiral invariance that restores standard electrodynamics. Astrophysical consequences of all these phenomena are discussed.Comment: Submitted to the 26th International Conference on High Energy Physics (using macropackage REVTEX II), 10 page

Proton $\beta% decay in large magnetic fields

A delicate interplay between the anomalous magnetic moments of the proton and neutron makes, in magnetic fields $B\ge 2\times 10^{14}$ T, the neutron stable and for fields $B\ge 5\times 10^{14}$ T the proton becomes unstable to a decay into a neutron via $\beta$ emission. Limits on the field strengths for which these arguments hold are presented and are related to questions of vacuum stability in the presence of such fields. Possible astrophysical consequences are discussed.Comment: 12 page

Dependence of Lattice Hadron Masses on External Magnetic Fields

We study the variation of the hadron masses in the presence of external magnetic fields of strength of the order of the masses themselves. We identify the main factors affecting the lattice simulation results: - the boundary discontinuities for $eB << 2\pi / L^2 a^2$. - the SU(6) choice of the hadron wave-function. We confirm qualitatively the earlier theoretical ansatz on the linear behaviour of the masses with the magnetic field and, as a by-product, we improve the lattice measurements of the nucleon magnetic moments. However our systematic and statistical errors preclude us from measuring the theoretically predicted field strength at which the proton becomes heavier than the neutron.Comment: 18 pages, compressed uuencoded postscript fil

Baryon Mass Splittings in the 1/N_c Expansion

The $I=0,1,2,3$ mass splittings of the spin-$1/2$ octet and spin-$3/2$ decuplet baryons are analyzed in the $1/\N$ expansion combined with perturbative flavor breaking. We show there is considerable experimental evidence that the baryon masses satisfy the hierarchy predicted by this expansion. Since flavor symmetry-breaking suppression factors alone are not sufficient to describe the observed hierarchy, we conclude that there is firm evidence for the $1/\N$ expansion in the baryon masses. Our analysis differs from non-relativistic $SU(6)$.Comment: 17 pages, LaTe

NON PERTURBATIVE EFFECTS AND QCD SUM RULES

No abstract availabl

SPIN AND QUARK MASS EFFECTS IN QCD SPECTROSCOPY

Les forces de spin dépendent de la saveur. Elles induisent ainsi des effets importants à travers la brisure chirale. La brisure d'isospin peut aussi être importante. En utilisant des méthodes basées sur la QCD, nous discutons un certain nombre d'effets qui sont non négligeables et qui peuvent être mesurés à LEAR.Spin forces are flavour dependent. They also induce large effects through chiral breaking. Isospin breaking also can be large. We discuss using QCD methods a variety of effects that are large and can be measured at LEAR

The status of QCD: Implications for cosmic rays

SIGLECopy held by FIZ Karlsruhe; available from UB/TIB Hannover / FIZ - Fachinformationszzentrum Karlsruhe / TIB - Technische InformationsbibliothekDEGerman