Correction to “Magnetic potential and magnetization contrasts of Earth's lithosphere” by J. Arkani‐Hamed and J. Dyment

Abstract

The term 6.., was typed y.., by mistake. Definitions of ¾nm and 6.m are given in equations (19a) and (19b) of the paper.

Tidal instability in exoplanetary systems evolution

“…The tidal instability is expected to be dynamo capable, as already suggested in Malkus (1993), Lacaze et al (2006) or Arkani-Hamed et al (2008). In this case, the magnetic field dynamics should be very different from the dynamics driven by a thermo-solutal convective dynamo.…”

Small numbers in supersymmetric theories of nature

“…Typically, I'~ae~m N O.Olm so that x w 1 if (Am)/m~0.01. This is close to the upper bound from the p + e~limit, so there could be a suppression due to either x or sin O [51,52]. It is possible, however, that for a specific SUSY spectrum the decay width could be much smaller than this naive estimate, allowing for a larger range of Am/m consistent with the rare decay limit (even for large mixing angles) and x N 1 so that the oscillation signal is not suppressed 1.…”

“…The chargino background can also be eliminated in considering a flavor violating and CP violating dilepton signal [52]. The presence of non-trivial phases in the slepton mixing matrix W breaks C'P, and results in a non-vanishing asymmetry: lV(e+p--e-p+) # O.…”

“…(4.2) (say in association with an electron). Since~(a = 1) is not a mass eigenstate, there is a probability that as it propagates it will convert to a F (o = 2) and hence decay into a p [51,52]:…”

“…at the LHC and NLC were studied in [52]. At a hadron collider (the sleptons can be pair-produced by the Drell-Yan process giving the same This was studied in [53,54], and is a promising signaI for large flavor mixing angles and when the SUSY background is known to be smz 11.…”