255,572 research outputs found
couplings and D^*\rar D\pi(\gamma) -decays within a -expansion in QCD
To leading order in , we evaluate the leading and non-leading
corrections to the and couplings using QCD
spectral moment sum rules in the full theory. We find that, for large and
contrary to the heavy-to-light B\rar \pi(\rho) l\bar \nu form factors, which
are dominated by the light quark vacuum condensate, these couplings are
governed by the perturbative graph, like other heavy-to-heavy
transitions. We also find that for the B^{*}\rar B\gamma, the
correction is mainly due to the perturbative and light quark condensate
contributions originating from the graphs involving the heavy quark part of the
electromagnetic current, which are essential for explaining the large charge
dependence in the observed D^{*-}\rar D^-\gamma and D^{*0}\rar D^0\gamma
decays. Our numerical predictions {\it without any free parameters} for
the -meson are: , \Gamma_{B^{*-}\rar
B^-\gamma}\simeq (0.10\pm 0.03) keV and the large charge dependence of the
ratio: {\Gamma_{B^{*-}\rar B^- \gamma}}/ {\Gamma_{B^{*0}\rar B^0
\gamma}}\simeq 2.5~. For the -meson, we find: \Gamma_{D^{*-}\rar
D^0\pi^-}\simeq 1.54\Gamma_{D^{*0}\rar D^0\pi^0} \simeq (8\pm 5) keV,
\Gamma_{D^{*-}\rar D^-\gamma}\simeq (0.09^{+0.40}_{-0.07} ) keV and
\Gamma_{D^{*0}\rar D^0\gamma}\simeq (3.7\pm 1.2) keV, where the branching
ratios agree within the errors with the present data, while the total widths
\Gamma_{D^{*0}\rar all} \simeq (11\pm 4) keV and \Gamma_{D^{*-}\rar
all}\simeq (12\pm 7) keV are much smaller than the present experimental upper
limits.Comment: published version to appear in Phys. Lett. B (minor modifications
compared with the previous version
Observation of the decay \psip\rar\kstark
Using 14 million events collected with the BESII detector,
branching fractions of \psip\rar\kstarkpm and \kstarknn are determined to
be: \calB(\psip\rar\kstarkpm)=(2.9^{+1.3}_{-1.7}\pm0.4)\times 10^{-5} and
\calB(\psip\rar\kstarknn)=(13.3^{+2.4}_{-2.7}\pm1.9)\times 10^{-5}. The
results confirm the violation of the "12%" rule for these two decay channels
with higher precision. A large isospin violation between the charged and
neutral modes is observed.Comment: 5 pages, 3 figure
A coordinated phosphorylation cascade initiated by MSK1 directs RAR alpha recruitment to target gene promoters
The nuclear retinoic acid (RA) receptor alpha (RARα) is a transcriptional transregulator that controls the expression of specific gene subsets through binding at response elements and dynamic interactions with coregulators, which are coordinated by the ligand. Here, we highlighted a novel paradigm in which the transcription of RARα-target genes is controlled by phosphorylation cascades initiated by the rapid RA activation of the p38MAPK/MSK1 pathway. We demonstrate that MSK1 phosphorylates RARα at S369 located in the Ligand Binding Domain, allowing the binding of TFIIH and thereby phosphorylation of the N-terminal domain at S77 by cdk7/cyclin H. MSK1 also phosphorylates Histone H3 at S10. Finally, the phosphorylation cascade initiated by MSK1 is required for the recruitment of RARα/TFIIH complexes to response elements and subsequently for RARα target genes activation. Cancer cells characterized by a deregulated p38MAPK/MSK1 pathway, do not respond to RA, outlining the essential contribution of the RA-triggered phosphorylation cascade in RA signaling
A hydrogenic molecular atmosphere of a neutron star
A model of a hydrogenic content of atmosphere of the isolated neutron star
1E1207.4-5209 is proposed. It is based on the assumption that the main
component in the atmosphere is the exotic molecular ion and that
there exists a magnetic field in the range of G.
Photoionization H_3^{2+} \rar e + 3p and photodissociation H_3^{2+} \rar H +
2p correspond to two absorption features at 0.7 KeV and 1.4 KeV, respectively,
discovered by {\it Chandra} observatory (Sanwal et al, 2002). The model
predicts one more absorption feature at 80-150 eV corresponding to
photodissociation H_3^{2+} \rar H_2^+ + p.Comment: 8 pages, 1 figur
The radial acceleration relation is a natural consequence of the baryonic Tully-Fisher relation
Galaxies covering several orders of magnitude in stellar mass and a variety
of Hubble types have been shown to follow the "Radial Acceleration Relation"
(RAR), a relationship between , the observed circular acceleration
of the galaxy, and , the acceleration due to the total baryonic
mass of the galaxy. For accelerations above ,
traces , asymptoting to the 1:1 line. Below this
scale, there is a break in the relation such that . We show that the RAR slope, scatter and the acceleration scale are
all natural consequences of the well-known baryonic Tully-Fisher relation
(BTFR). We further demonstrate that galaxies with a variety of baryonic and
dark matter (DM) profiles and a wide range of dark halo and galaxy properties
(well beyond those expected in CDM) lie on the RAR if we simply require that
their rotation curves satisfy the BTFR. We explore conditions needed to break
this degeneracy: sub-kpc resolved rotation curves inside of "cored"
DM-dominated profiles and/or outside kpc could lie on BTFR but
deviate in the RAR, providing new constraints on DM.Comment: 5 pages, submitted to MNRA
Dominance of the light-quark condensate in the heavy-to-light exclusive decays
Using the QCD {\it hybrid} (moments-Laplace) sum rule, we show
- that, in the limit M_b \rar \infty, the and
behaviours of the heavy-to-light exclusive (\bar B\rar \rho~(\pi)
semileptonic as well as the B\rar \rho\gamma rare) decay--form factors are
dominated by the contribution of the soft light-quark condensate
rather than that of the hard perturbative diagram. The QCD-analytic
behaviour of the form factors is a polynomial in , which mimics
quite well the usual pole parametrization, except in the case of the
form factor, where there is a significant deviation from this polar form. The
-dependence of the form factors expected from HQET and lattice results is
recovered. We extract with a good accuracy the ratios: , and ; combined with the ``world average" value of or/and
, these ratios lead to the decay rates: $\Gamma_{\bar B\rar \pi e\bar
\nu} \simeq (4.3 \pm 0.7)Comment: 10 pages, CERN-TH 7237/94 (the previous version contains numerical
errors). Latex file (run twice) 3 ps.figures available by mai
Retinoic Acid Receptor Overexpression in Human Umbilical Cord-derived Mesenchymal Stem Cells
Introduction: Retinoic acid (RA) involves in vertebrate morphogenesis, growth and apoptosis through two classes of receptors encoded by six genes; RAR, and RXR, . The former utilizes either all-trans RA or 9-cis-RA as ligands, whereas the RXRs utilize only 9-cis-RA. Using the human umbilical cord derived stem cells (HUCSCs) as an in vitro model of human fetal cells we aimed to evaluate RAR overexpression following to RA treatment.
Methods: HUCSCs were cultured in DMEM + 10% FBS at a density of 1 × 103/ well. Upon adhering, the medium was changed to DMEM containing RA for 4-6 days during which RA refreshed every 2 days. The untreated cells were considered as a control group. Using a combination of flowcytometry, MTT colorimetric assay and conventional RT-PCR techniques, CD markers, cell viability and RAR expression profile of HUCSCs were measured, respectively.
Results: Flowcytometry analysis clearly indicated 5.4% of HUCSCs co-expressed CD34 and CD45, while 63.7% of cells expressed both CD44 and CD73. 36.5% of cells expressed CD90 compared to 0.05% for CD105.MTT assay also showed that about 60% of HUCSCsˈ viability decreased at higher doses (10-7 – 10-5M) of RA compared to control group. RT-PCR analysis also revealed that RAR and were upregulated in the RA–treated cells.
Conclusions: This study clearly shows that the HUCSCs express CD44, CD73 and CD90 and RA in a dose-dependent manner has a cytotoxicity effect on HUCSCs that is mediated by RAR an
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