164 research outputs found
A Long Baseline Neutrino Oscillation Experiment Using J-PARC Neutrino Beam and Hyper-Kamiokande
Document submitted to 18th J-PARC PAC meeting in May 2014. 50 pages, 41 figuresDocument submitted to 18th J-PARC PAC meeting in May 2014. 50 pages, 41 figuresDocument submitted to 18th J-PARC PAC meeting in May 2014. 50 pages, 41 figuresHyper-Kamiokande will be a next generation underground water Cherenkov detector with a total (fiducial) mass of 0.99 (0.56) million metric tons, approximately 20 (25) times larger than that of Super-Kamiokande. One of the main goals of Hyper-Kamiokande is the study of asymmetry in the lepton sector using accelerator neutrino and anti-neutrino beams. In this document, the physics potential of a long baseline neutrino experiment using the Hyper-Kamiokande detector and a neutrino beam from the J-PARC proton synchrotron is presented. The analysis has been updated from the previous Letter of Intent [K. Abe et al., arXiv:1109.3262 [hep-ex]], based on the experience gained from the ongoing T2K experiment. With a total exposure of 7.5 MW 10 sec integrated proton beam power (corresponding to protons on target with a 30 GeV proton beam) to a -degree off-axis neutrino beam produced by the J-PARC proton synchrotron, it is expected that the phase can be determined to better than 19 degrees for all possible values of , and violation can be established with a statistical significance of more than () for () of the parameter space
ĐŃĐŸĐ±Đ»ĐžĐČĐŸŃŃŃ ŃĐŸŃĐŒŃĐČĐ°ĐœĐœŃ ŃĐ°ĐŒĐŸŃŃŃĐčĐœĐŸŃ ĐżŃĐ·ĐœĐ°ĐČĐ°Đ»ŃĐœĐŸŃ ĐŽŃŃĐ»ŃĐœĐŸŃŃŃ ĐŒĐ°ĐčбŃŃĐœŃŃ ŃŃĐžŃДлŃĐČ ĐŒĐ°ŃĐ”ĐŒĐ°ŃĐžĐșĐž
(uk) ĐŁ ŃŃĐ°ŃŃŃ Đ·ŃĐŸĐ±Đ»Đ”ĐœĐŸ ŃĐżŃĐŸĐ±Ń ŃĐŸĐ·ĐșŃĐžŃĐž ĐŸŃĐŸĐ±Đ»ĐžĐČĐŸŃŃŃ ŃĐ°ĐŒĐŸŃŃŃĐčĐœĐŸŃ ĐżŃĐ·ĐœĐ°ĐČĐ°Đ»ŃĐœĐŸŃ ĐŽŃŃĐ»ŃĐœĐŸŃŃŃ ĐŒĐ°ĐčбŃŃĐœŃŃ
ĐČŃĐžŃДлŃĐČ; ĐŽĐŸŃĐ»ŃЎжŃŃŃŃŃŃ ŃŃĐ·ĐœŃ ĐżŃĐŽŃ
ĐŸĐŽĐž ĐŽĐŸ ŃŃĐŸĐłĐŸ ĐżĐŸĐœŃŃŃŃ; ŃĐŸĐ·ĐșŃĐžĐČĐ°ŃŃŃŃŃ ŃĐ°ĐșŃ ĐčĐŸĐłĐŸ ŃĐșĐ»Đ°ĐŽĐŸĐČŃ, ŃĐș ŃĐ°ĐŒĐŸŃŃŃĐčĐœŃŃŃŃ, ĐżŃĐ·ĐœĐ°ĐČĐ°Đ»ŃĐœĐ° ŃĐ°ĐŒĐŸŃŃŃĐčĐœŃŃŃŃ, ĐżŃĐ·ĐœĐ°ĐČĐ°Đ»ŃĐœĐ° ĐŽŃŃĐ»ŃĐœŃŃŃŃ.(ru) Đ ŃŃĐ°ŃŃĐ” ŃĐŽĐ”Đ»Đ°ĐœĐ° ĐżĐŸĐżŃŃĐșĐ° ŃĐ°ŃĐșŃŃŃŃ ĐŸŃĐŸĐ±Đ”ĐœĐœĐŸŃŃĐž ŃĐ°ĐŒĐŸŃŃĐŸŃŃДлŃĐœĐŸĐč ĐżĐŸĐ·ĐœĐ°ĐČĐ°ŃДлŃĐœĐŸĐč ĐŽĐ”ŃŃДлŃĐœĐŸŃŃĐž бŃĐŽŃŃĐžŃ
ŃŃĐžŃДлДĐč; ĐžŃŃлДЎŃŃŃŃŃ ŃазлОŃĐœŃĐ” ĐżĐŸĐŽŃ
ĐŸĐŽŃ Đș ŃŃĐŸĐŒŃ ĐżĐŸĐœŃŃĐžŃ; ŃĐ°ŃĐșŃŃĐČĐ°ŃŃŃŃ ŃĐ°ĐșОД Đ”ĐłĐŸ ŃĐŸŃŃĐ°ĐČĐ»ŃŃŃОД, ĐșĐ°Đș ŃĐ°ĐŒĐŸŃŃĐŸŃŃДлŃĐœĐŸŃŃŃ, ĐżĐŸĐ·ĐœĐ°ĐČĐ°ŃДлŃĐœĐ°Ń ŃĐ°ĐŒĐŸŃŃĐŸŃŃДлŃĐœĐŸŃŃŃ, ĐżĐŸĐ·ĐœĐ°ĐČĐ°ŃДлŃĐœĐ°Ń ĐŽĐ”ŃŃДлŃĐœĐŸŃŃŃ
Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with 6.6 x 10(20) protons on target
111 pages, 45 figures, submitted to Physical Review D. Minor revisions to text following referee comments111 pages, 45 figures, submitted to Physical Review D. Minor revisions to text following referee comments111 pages, 45 figures, submitted to Physical Review D. Minor revisions to text following referee commentsWe thank the J-PARC staff for superb accelerator performance and the CERN NA61/SHINE Collaboration for providing valuable particle production data. We acknowledge the support of MEXT, Japan; NSERC, NRC, and CFI, Canada; CEA and CNRS/IN2P3, France; DFG, Germany; INFN, Italy; National Science Centre (NCN), Poland; RSF, RFBR and MES, Russia; MINECO and ERDF funds, Spain; SNSF and SER, Switzerland; STFC, UK; and the U. S. Deparment of Energy, USA. We also thank CERN for the UA1/NOMAD magnet, DESY for the HERA-B magnet mover system, NII for SINET4, the WestGrid and SciNet consortia in Compute Canada, GridPP, UK, and the Emerald High Performance Computing facility in the Centre for Innovation, UK. In addition, participation of individual researchers and institutions has been further supported by funds from ERC (FP7), EU; JSPS, Japan; Royal Society, UK; and DOE Early Career program, USA
Measurement of the electron neutrino charged-current interaction rate on water with the T2K ND280 pi(0) detector
10 pages, 6 figures, Submitted to PRDhttp://journals.aps.org/prd/abstract/10.1103/PhysRevD.91.112010© 2015 American Physical Society11 pages, 6 figures, as accepted to PRD11 pages, 6 figures, as accepted to PRD11 pages, 6 figures, as accepted to PR
Comparative analysis of involvement of UGT1 and UGT2 splice variants of UDP-galactose transporter in glycosylation of macromolecules in MDCK and CHO cell lines
Nucleotide sugar transporters deliver nucleotide sugars into the Golgi apparatus and endoplasmic reticulum. This study aimed to further characterize mammalian UDP-galactose transporter (UGT) in MDCK and CHO cell lines. MDCK-RCAr and CHO-Lec8 mutant cell lines are defective in UGT transporter, although they exhibit some level of galactosylation. Previously, only single forms of UGT were identified in both cell lines, UGT1 in MDCK cells and UGT2 in CHO cells. We have identified the second UGT splice variants in CHO (UGT1) and MDCK (UGT2) cells. Compared to UGT1, UGT2 is more abundant in nearly all examined mammalian tissues and cell lines, but MDCK cells exhibit different relative distribution of both splice variants. Complementation analysis demonstrated that both UGT splice variants are necessary for N- and O-glycosylation of proteins. Both mutant cell lines produce chondroitin-4-sulfate at only a slightly lower level compared to wild-type cells. This defect is corrected by overexpression of both UGT splice variants. MDCK-RCAr mutant cells do not produce keratan sulfate and this effect is not corrected by either UGT splice variant, overexpressed either singly or in combination. Here we demonstrate that both UGT splice variants are important for glycosylation of proteins. In contrast to MDCK cells, MDCK-RCAr mutant cells may possess an additional defect within the keratan sulfate biosynthesis pathway
RANKL Is a Downstream Mediator for Insulin-Induced Osteoblastic Differentiation of Vascular Smooth Muscle Cells
Several reports have shown that circulating insulin level is positively correlated with arterial calcification; however, the relationship between insulin and arterial calcification remains controversial and the mechanism involved is still unclear. We used calcifying vascular smooth muscle cells (CVSMCs), a specific subpopulation of vascular smooth muscle cells that could spontaneously express osteoblastic phenotype genes and form calcification nodules, to investigate the effect of insulin on osteoblastic differentiation of CVSMCs and the cell signals involved. Our experiments demonstrated that insulin could promote alkaline phosphatase (ALP) activity, osteocalcin expression and the formation of mineralized nodules in CVSMCs. Suppression of receptor activator of nuclear factor ÎșB ligand (RANKL) with small interfering RNA (siRNA) abolished the insulin-induced ALP activity. Insulin induced the activation of extracellular signal-regulated kinase (ERK)1/2, mitogen-activated protein kinase (MAPK) and RAC-alpha serine/threonine-protein kinase (Akt). Furthermore, pretreatment of human osteoblasts with the ERK1/2 inhibitor PD98059, but not the phosphoinositide 3-kinase (PI3K) inhibitor, LY294002, or the Akt inhibitor, 1L-6-hydroxymethyl-chiro-inositol 2-(R)-2-O-methyl-3-O-octadecylcarbonate (HIMO), abolished the insulin-induced RANKL secretion and blocked the promoting effect of insulin on ALP activities of CVSMCs. Recombinant RANKL protein recovered the ALP activities decreased by RANKL siRNA in insulin-stimulated CVSMCs. These data demonstrated that insulin could promote osteoblastic differentiation of CVSMCs by increased RANKL expression through ERK1/2 activation, but not PI3K/Akt activation
Pharmacogenetic & Pharmacokinetic Biomarker for Efavirenz Based ARV and Rifampicin Based Anti-TB Drug Induced Liver Injury in TB-HIV Infected Patients
BACKGROUND: Implication of pharmacogenetic variations and efavirenz pharmacokinetics in concomitant efavirenz based antiviral therapy and anti-tubercular drug induced liver injury (DILI) has not been yet studied. We performed a prospective case-control association study to identify the incidence, pharmacogenetic, pharmacokinetic and biochemical predictors for anti-tubercular and antiretroviral drugs induced liver injury (DILI) in HIV and tuberculosis (TB) co-infected patients. METHODS AND FINDINGS: Newly diagnosed treatment naĂŻve TB-HIV co-infected patients (nâ=â353) were enrolled to receive efavirenz based ART and rifampicin based anti-TB therapy, and assessed clinically and biochemically for DILI up to 56 weeks. Quantification of plasma efavirenz and 8-hydroxyefaviernz levels and genotyping for NAT2, CYP2B6, CYP3A5, ABCB1, UGT2B7 and SLCO1B1 genes were done. The incidence of DILI and identification of predictors was evaluated using survival analysis and the Cox Proportional Hazards Model. The incidence of DILI was 30.0%, or 14.5 per 1000 person-week, and that of severe was 18.4%, or 7.49 per 1000 person-week. A statistically significant association of DILI with being of the female sex (pâ=â0.001), higher plasma efavirenz level (pâ=â0.009), efavirenz/8-hydroxyefavirenz ratio (pâ=â0.036), baseline AST (pâ=â0.022), ALT (pâ=â0.014), lower hemoglobin (pâ=â0.008), and serum albumin (pâ=â0.007), NAT2 slow-acetylator genotype (pâ=â0.039) and ABCB1 3435TT genotype (pâ=â0.001). CONCLUSION: We report high incidence of anti-tubercular and antiretroviral DILI in Ethiopian patients. Between patient variability in systemic efavirenz exposure and pharmacogenetic variations in NAT2, CYP2B6 and ABCB1 genes determines susceptibility to DILI in TB-HIV co-infected patients. Close monitoring of plasma efavirenz level and liver enzymes during early therapy and/or genotyping practice in HIV clinics is recommended for early identification of patients at risk of DILI
Metal-Poor Stars and the Chemical Enrichment of the Universe
Metal-poor stars hold the key to our understanding of the origin of the
elements and the chemical evolution of the Universe. This chapter describes the
process of discovery of these rare stars, the manner in which their surface
abundances (produced in supernovae and other evolved stars) are determined from
the analysis of their spectra, and the interpretation of their abundance
patterns to elucidate questions of origin and evolution. More generally,
studies of these stars contribute to other fundamental areas that include
nuclear astrophysics, conditions at the earliest times, the nature of the first
stars, and the formation and evolution of galaxies -- including our own Milky
Way. We illustrate this with results from studies of lithium formed during the
Big Bang; of stars dated to within ~1 Gyr of that event; of the most metal-poor
stars, with abundance signatures very different from all other stars; and of
the build-up of the elements over the first several Gyr. The combination of
abundance and kinematic signatures constrains how the Milky Way formed, while
recent discoveries of extremely metal-poor stars in the Milky Way's dwarf
galaxy satellites constrain the hierarchical build-up of its stellar halo from
small dark-matter dominated systems. [abridged]Comment: Book chapter, emulated version, 34 pages; number of references are
limited by publisher; to appear in Vol. 5 of textbook "Planets, Stars and
Stellar Systems", by Springer, in 201
Sensitivity of the T2K accelerator-based neutrino experiment with an Extended run to POT
18 pages, 4 figures18 pages, 4 figures18 pages, 4 figures18 pages, 4 figures18 pages, 4 figuresRecent measurements at the T2K experiment indicate that CP violation in neutrino mixing may be observed in the future by long-baseline neutrino oscillation experiments. We explore the physics program of an extension to the currently approved T2K running of protons-on-target to protons-on-target,aiming at initial observation of CP violation with 3 or higher significance for the case of maximum CP violation. With accelerator and beam line upgrades, as well as analysis improvements, this program would occur before the next generation of long-baseline neutrino oscillation experiments that are expected to start operation in 2026.We acknowledge the support of MEXT, Japan; NSERC (Grant No. SAPPJ-2014-00031), NRC and CFI, Canada; CEA and CNRS/IN2P3, France; DFG, Germany; INFN, Italy; National Science Centre (NCN), Poland; RSF, RFBR and MES, Russia; MINECO and ERDF funds, Spain; SNSF and SERI, Switzerland; STFC, UK; and DOE, USA. We also thank CERN for the UA1/NOMAD magnet, DESY for the HERA-B magnet mover system, NII for SINET4, the WestGrid and SciNet consortia in Compute Canada, and GridPP in the United Kingdom. In addition, participation of individual researchers and institutions has been further supported by funds from ERC (FP7), H2020 Grant No. RISE-GA644294-JENNIFER, EU; JSPS, Japan; Royal Society, UK; and the DOE Early Career program, USA. CNRS/IN2P3: Centre National de la Recherche ScientifiqueInstitut National de Physique Nucleaire et de Physique des Particules RSF: Russian Science Foundation MES: Ministry of Education and Science, Russia ERDF: European Regional Development Fund SNSF: Swiss National Science Foundation SER (should be SERI): State Secretariat for Education, Research and Innovatio
Precise Measurement of the Neutrino Mixing Parameter theta(23) from Muon Neutrino Disappearance in an Off-Axis Beam
New data from the T2K neutrino oscillation experiment produce the most precise measurement of the neutrino mixing parameter theta_{23}. Using an off-axis neutrino beam with a peak energy of 0.6 GeV and a data set corresponding to 6.57 x 10^{20} protons on target, T2K has fit the energy-dependent nu_mu oscillation probability to determine oscillation parameters. Marginalizing over the values of other oscillation parameters yields sin^2 (theta_{23}) = 0.514 +0.055/-0.056 (0.511 +- 0.055), assuming normal (inverted) mass hierarchy. The best-fit mass-squared splitting for normal hierarchy is Delta m^2_{32} = (2.51 +- 0.10) x 10^{-3} eV^2/c^4 (inverted hierarchy: Delta m^2_{13} = (2.48 +- 0.10) x 10^{-3} eV^2/c^4). Adding a model of multinucleon interactions that affect neutrino energy reconstruction is found to produce only small biases in neutrino oscillation parameter extraction at current levels of statistical uncertainty
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