19,019,109 research outputs found
Exclusive B -> pi e^+ e^- and B -> rho e^+ e^-
We investigate the exclusive B -> pi e^+ e^- and B -> rho e^+ e^- decays in
framework of the general two Higgs doublet model (model III), in which an extra
phase angle in the charged--Higgs fermion coupling, i.e., a new source for CP
violation exists. The CP violation for both decays are calculated and it is
observed that the CP violating asymmetry in model III differs significantly
than the one predicted by the standard model and model II which is a special
case of model III. Furthermore, it is shown that the zero value of forward
backward asymmetry A_{FB} is shifted when compared with the SM value, which can
also serve as the efficiency tool for establishing new physics.Comment: 21 pages, 8 figures, 4 Tables LaTeX formatte
Determining V(ub) from B+ --> D*+(s) e+ e- and B+ --> D*+ e+ e-
It was recently pointed out that the decays B^+ --> D^{*+}_s gamma and B^+
--> D^{*+} gamma can be used for an extraction of |V_{ub}|. The theory of these
decays is poorly understood. It was shown that in a world of almost degenerate
b and c-quarks the decay would be computable. The severe difficulties that are
encountered in the realistic calculation stem primarily from the very hard
photon produced in the two body decay. We point out that in the decays B^+ -->
D^{*+}_s e^+e^- and B^+ --> D^{*+} e^+e^- the photon vertex is soft when the
charmed meson is nearly at rest (in the B^+ rest frame). This allows us to
compute with some confidence the decay rate in a restricted but interesting
kinematic regime. Given enough data the extraction of V_{ub} with reasonably
small uncertainties could proceed through an analysis of these exclusive decays
much as is done in the determination of V_{cb}.Comment: 9 pages, latex (revtex), replaced with published versio
Operator Product Expansion for Exclusive Decays: B^+ ->Ds^+ e+e- and B^+ -> Ds^{*+} e+e-
The decays and proceed
through a weak and an electromagnetic interaction. This is a typical ``long
distance'' process, usually difficult to compute systematically. We propose
that over a large fraction of phase space a combination of an operator product
and heavy quark expansions effectively turns this process into one in which the
weak and electromagnetic interactions occur through a local operator. Moreover,
we use heavy quark spin symmetry to relate all the local operators that appear
in leading order of the operator expansion to two basic ones. We use this
operator expansion to estimate the decay rates for .Comment: 4 pages, 1 figure, Latex, published version in PR
Measurement of the running b-quark mass using events
We have studied the determination of the running b-quark mass, ,
using decays into 3 or more hadronic jets. We calculated the ratio of
-jet fractions in vs.
( = u or d or s) events at next-to-leading order in perturbative QCD using
six different infra-red- and collinear-safe jet-finding algorithms. We compared
with corresponding measurements from the SLD Collaboration and found a
significant algorithm-dependence of the fitted value. Our best
estimate, taking correlations into account, is .Comment: 22 pages (LaTeX), 1 Postscript figure. Version to appear in Phys.
Lett. B. Several clarifying remarks added in the text, typos corrected, and
theoretical results for very small masses added in the figur
HIGGS BOSON PRODUCTION IN
The production of the Standard Model Higgs boson in the four-fermion reaction
is studied. The complete tree-level matrix
element, including signal and backgrounds in the standard electroweak theory,
is computed and initial state radiation is taken into account in the
leading-log approximation. A Monte Carlo event generator has been built and
numerical results for some distributions of experimental interest for the
search of the Higgs particle at future electron-positron colliders are shown,
compared with those existing in the literature and commented.Comment: 8 pages, 5 figures available via anonymous ftp at:
ftp://cobra1.pv.infn.it/pub/4f/, files fig#h.ps with #=1,...,5
Extended shells around B[e] stars - implications for B[e] star evolution
Aims. The position of B[e] stars in the upper left part of the Hertzsprung-Russell diagram creates a quandary. Are these stars young stars evolving onto the main sequence or old stars that are evolving off of it? Spectral characteristics suggest that B[e] stars can be
placed into five subclasses and are not a homogeneous set. Such sub-classification is believed to coincide with varying origins and different evolutions. However, the evolutionary connection of B[e] stars – and notably sgB[e] – to other stars is unclear, particularly to evolved massive stars. We attempt to provide insight into the evolutionary past of B[e] stars.
Methods. We performed an Hα narrow-band CCD imaging survey of B[e] stars, in the northern hemisphere. Prior to the current work, no emission-line survey of B[e] stars had yet been made, while only two B[e] stars appeared to have a shell nebula as seen in the Digital Sky Survey. Of nebulae around B[e] stars, only the ring nebula around MWC137 has been previously observed extensively.
Results. In this presentation we report the findings from our narrow-band optical imaging survey of the environments of 25 B[e] stars. Of the objects surveyed, 7 show bipolar or uni- polar structures up to 15' across; 5 show faint, large, or filamentary shells; and 2 are compact planetary nebula-type systems. The most spectacular system observed is a large bipolar structure associated with MWC314.
Conclusions. The possible links between B[e] stars and other evolved stars, implied by our observations, are investigated
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