ar X iv : c s . IT / 0 51 11 03 v 1 3 0 N ov 2 00 5 An Infeasibility Result for the Multiterminal Source - Coding Problem ∗

ar X iv : a st ro - p h / 03 11 59 5 v 1 2 6 N ov 2 00 3 WHAT ARE S 0 ( 0 ) GALAXIES ?

Received ; accepted – 2 – ABSTRACT Among early-type galaxies with almost circular isophotes E0 and E1 galaxies are, at 99.3% significance, more luminous than face-on objects classified as S0 (0) and S(0) (1). This result supports the view that rotation and " diskiness " are more important in the outer regions of faint early-type galaxies than they are for more luminous galaxies of very early mo...

ar X iv : m at h / 03 11 30 1 v 1 [ m at h . N T ] 1 8 N ov 2 00 3 ON THE ESTIMATION OF Z 2 ( s ) Aleksandar

Estimates for Z2(s) = ∫∞ 1 |ζ(12 + ix)|4x−s dx (Re s > 1) are discussed, both pointwise and in the mean square. It is shown how these estimates can be used to bound E2(T ), the error term in the asymptotic formula for ∫ T 0 |ζ(12 + it)|4 dt.

ar X iv : g r - qc / 0 51 11 52 v 1 2 9 N ov 2 00 5 Recent results on the search for continuous sources with LIGO and GEO 600 Alicia

An overview of the searches for continuous gravitational wave signals in LIGO and GEO 600 performed on different recent science runs and results are presented. This includes both searching for gravitational waves from known pulsars as well as blind searches over a wide parameter space.

ar X iv : h ep - l at / 0 11 00 06 v 3 6 N ov 2 00 1 1 Matrix elements of ∆ S = 2 operators with Wilson fermions

ar X iv : h ep - p h / 03 11 17 0 v 1 1 3 N ov 2 00 3 Learning the weak phase γ from B decays Jonathan

The current status of some methods to determine the weak phase γ of the Cabibbo-Kobayashi-Maskawa (CKM) matrix element V ∗ ub using B decays is discussed, and comments are made on accuracy achievable in the next few years.