172 research outputs found
Near-Infrared Imaging of the Central Regions of Metal-Poor Inner Spheroid Globular Clusters
JHK images obtained with the Canada-France-Hawaii Telescope (CFHT) Adaptive
Optics Bonnette (AOB) are used to investigate the near-infrared photometric
properties of red giant branch (RGB) and horizontal branch (HB) stars in eight
metal-poor globular clusters with R_GC < 2 kpc. The slope of the RGB on the (K,
J-K) CMDs confirms the metal-poor nature of these clusters, four of which
appear to have metallicities comparable to M92. The luminosity functions of RGB
stars in inner spheroid and outer halo clusters have similar slopes, although
there is a tendency for core-collapsed clusters to have slightly flatter
luminosity functions than non-collapsed clusters. The distribution of red HB
stars on the (K, J-K) CMDs of inner spheroid clusters with [Fe/H] ~ -1.5 is
very different from that of clusters with [Fe/H] ~ -2.2, suggesting that
metallicity is the main parameter defining HB content among these objects. The
RGB-bump is detected in four of the inner spheroid clusters, and this feature
is used to compute distances to these objects. Finally, the specific frequency
of globular clusters in the inner Galaxy is discussed in the context of the
early evolution of the bulge. If the globular cluster formation efficiency for
the inner Galaxy is similar to that measured in other spheroidal systems, then
the main body of the bulge could have formed from gas that was chemically
enriched in situ.Comment: 26 pages of text and 13 postscript figures. To appear in the
Astronomical Journa
PEN: a low energy test of lepton universality
Allowed charged meson decays are characterized by simple dynamics, few
available decay channels, mainly into leptons, and extremely well controlled
radiative and loop corrections. In that sense, pion decays represent a
veritable triumph of the standard model (SM) of elementary particles and
interactions. This relative theoretical simplicity makes charged pion decays a
sensitive means for testing the underlying symmetries and the universality of
weak fermion couplings, as well as for studying pion structure and chiral
dynamics. Even after considerable recent improvements, experimental precision
is lagging far behind that of the theoretical description for pion decays. We
review the current state of experimental study of the pion electronic decay
, or , where the
indicates inclusion and explicit treatment of radiative decay events. We
briefly review the limits on non-SM processes arising from the present level of
experimental precision in decays. Focusing on the PEN
experiment at the Paul Scherrer Institute (PSI), Switzerland, we examine the
prospects for further improvement in the near term.Comment: 11 pages, 5 figures; paper presented at the XIII International
Conference on Heavy Quarks and Leptons, 22-27 May 2016, Blacksburg, Virginia,
US
PEN experiment: a precise measurement of the pi+ -> e+ nu decay branching fraction
A new measurement of , the decay
branching ratio, is currently under way at the Paul Scherrer Institute. The
present experimental result on constitutes the most accurate test
of lepton universality available. The accuracy, however, still lags behind the
theoretical precision by over an order of magnitude. Because of the large
helicity suppression of the decay, its branching ratio is
susceptible to significant contributions from new physics, making this decay a
particularly suitable subject of study.Comment: 4 pages, 3 figures, talk given at the Tenth Conference on the
Intersections of Particle and Nuclear Physics (CIPANP 2009), La Jolla/San
Diego, CA, 26-31 May 2009; to appear in Proceedings to be published by the
American Institute of Physic
Precise Measurement of the Pi+ -> Pi0 e+ nu Branching Ratio
Using a large acceptance calorimeter and a stopped pion beam we have made a
precise measurement of the rare Pi+ -> Pi0 e+ Nu,(pi_beta) decay branching
ratio. We have evaluated the branching ratio by normalizing the number of
observed pi_beta decays to the number of observed Pi+ -> e+ Nu, (pi_{e2})
decays. We find the value of Gamma(Pi+ -> Pi0 e+ Nu)/Gamma(total) = [1.036 +/-
0.004(stat.) +/- 0.004(syst.) +/- 0.003(pi_{e2})] x 10^{-8}$, where the first
uncertainty is statistical, the second systematic, and the third is the pi_{e2}
branching ratio uncertainty. Our result agrees well with the Standard Model
prediction.Comment: 4 pages, 5 figures, 1 table, revtex4; changed content; updated
analysi
Precise Measurement of pi+ -> e+ nu Branching Ratio
The PEN Collaboration is conducting a new measurement of the pi+ -> e+ nu
branching ratio at the Paul Scherrer Institute, with the goal uncertainty of
delta B/B(pie2)=5E-4 or lower. At present, the combined accuracy of all
published pie2 decay measurements lags behind the theoretical calculation by a
factor of 40. In this contribution we report on the PEN detector configuration
and its performance during two development runs done in 2007 and 2008.Comment: pdflatex, 11 pages, 5 figures, to be published in "Progress in
High-Energy Physics and Nuclear Safety", NATO Science for Peace Series: B -
Physics and Biophysic
Performance of the CMS Cathode Strip Chambers with Cosmic Rays
The Cathode Strip Chambers (CSCs) constitute the primary muon tracking device
in the CMS endcaps. Their performance has been evaluated using data taken
during a cosmic ray run in fall 2008. Measured noise levels are low, with the
number of noisy channels well below 1%. Coordinate resolution was measured for
all types of chambers, and fall in the range 47 microns to 243 microns. The
efficiencies for local charged track triggers, for hit and for segments
reconstruction were measured, and are above 99%. The timing resolution per
layer is approximately 5 ns
Precise Measurement of the Pion Axial Form Factor in the Pi+ -> e+ nu gamma Decay
We have studied radiative pion decays Pi+ -> e+ nu gamma in three broad
kinematic regions using the PIBETA detector and a stopped pion beam. Based on
Dalitz distributions of 42,209 events we have evaluated absolute Pi -> e nu
gamma branching ratios in the three regions. Minimum chi^2 fits to the integral
and differential (E(e+),E(gamma)) distributions result in the axial-to-vector
weak form factor ratio of gamma = F_A/F_V = 0.443(15),or F_A = 0.0115(4) with
F_V = 0.0259. However, deviations from Standard Model predictions in the
high-E(gamma)/low-E(e+) kinematic region indicate the need for further
theoretical and experimental work.Comment: 5 pages, 4 figures, 1 table, revtex
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