# United States Department of Energy High Energy Physics Division

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Works: 2,926 works in 2,977 publications in 1 language and 9,079 library holdings Conference papers and proceedings Sponsor, Researcher, Other
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High energy density and high power RF : 5th Workshop on High Energy Density and High Power RF : Snowbird, Utah, 1-5 October 2001 by Workshop on High Energy Density and High Power RF( Book )

2 editions published in 2002 in English and held by 110 WorldCat member libraries worldwide

The SDSS-IV extended Baryon Oscillation Spectroscopic Survey : Overview and early data( )

2 editions published in 2016 in English and held by 0 WorldCat member libraries worldwide

In a six-year program started in 2014 July, the Extended Baryon Oscillation Spectroscopic Survey (eBOSS) will conduct novel cosmological observations using the BOSS spectrograph at Apache Point Observatory. These observations will be conducted simultaneously with the Time Domain Spectroscopic Survey (TDSS) designed for variability studies and the Spectroscopic Identification of eROSITA Sources (SPIDERS) program designed for studies of X-ray sources. In particular, eBOSS will measure with percent-level precision the distance-redshift relation with baryon acoustic oscillations (BAO) in the clustering of matter. eBOSS will use four different tracers of the underlying matter density field to vastly expand the volume covered by BOSS and map the large-scale-structures over the relatively unconstrained redshift range 0.6 <z <2.2. Using more than 250,000 new, spectroscopically confirmed luminous red galaxies at a median redshift z = 0.72, we project that eBOSS will yield measurements of the angular diameter distance dA(z) to an accuracy of 1.2% and measurements of H(z) to 2.1% when combined with the z> 0.6 sample of BOSS galaxies. With ~195,000 new emission line galaxy redshifts, we expect BAO measurements of dA(z) to an accuracy of 3.1% and H(z) to 4.7% at an effective redshift of z = 0.87. A sample of more than 500,000 spectroscopically confirmed quasars will provide the first BAO distance measurements over the redshift range 0.9 <z <2.2, with expected precision of 2.8% and 4.2% on dA(z) and H(z), respectively. Finally, with 60,000 new quasars and re-observation of 60,000 BOSS quasars, we will obtain new Ly[alpha] forest measurements at redshifts z> 2.1; these new data will enhance the precision of dA(z) and H(z) at z> 2.1 by a factor of 1.44 relative to BOSS. Furthermore, eBOSS will provide improved tests of General Relativity on cosmological scales through redshift-space distortion measurements, improved tests for non-Gaussianity in the primordial density field, and new constraints on the summed mass of all neutrino species. Lastly, we provide an overview of the cosmological goals, spectroscopic target sample, demonstration of spectral quality from early data, and projected cosmological constraints from eBOSS
Automated Transient Identification in the Dark Energy Survey( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

We describe an algorithm for identifying point-source transients and moving objects on reference-subtracted optical images containing artifacts of processing and instrumentation. The algorithm makes use of the supervised machine learning technique known as Random Forest. We present results from its use in the Dark Energy Survey Supernova program (DES-SN), where it was trained using a sample of 898,963 signal and background events generated by the transient detection pipeline. After reprocessing the data collected during the first DES-SN observing season (2013 September through 2014 February) using the algorithm, the number of transient candidates eligible for human scanning decreased by a factor of 13.4, while only 1.0 percent of the artificial Type Ia supernovae (SNe) injected into search images to monitor survey efficiency were lost, most of which were very faint events. Here we characterize the algorithm's performance in detail, and we discuss how it can inform pipeline design decisions for future time-domain imaging surveys, such as the Large Synoptic Survey Telescope and the Zwicky Transient Facility
Effect of event selection on jetlike correlation measurement in [mml : math altimg="si1.gif" overflow="scroll" xmlns xocs="http //www.elsevier.com/xml/xocs/dtd" xmlns xs="http //www.w3.org/2001/XMLSchema" xmlns xsi="http //www.w3.org/2001/XMLSchema-instance" xmlns="http //www.elsevier.com/xml/ja/dtd" xmlns ja="http //www.elsevier.com/xml/ja/dtd" xmlns mml="http //www.w3.org/1998/Math/MathML" xmlns tb="http //www.elsevier.com/xml/common/table/dtd" xmlns sb="http //www.elsevier.com/xml/common/struct-bib/dtd" xmlns ce="http //www.elsevier.com/xml/common/dtd" xmlns xlink="http //www.w3.org/1999/xlink" xmlns cals="http //www.elsevier.com/xml/common/cals/dtd" xmlns sa="http //www.elsevier.com/xml/common/struct-aff/dtd"][mml mi]d[/mml mi][mml mo]+[/mml mo][mml mrow][mml mi mathvariant="normal"]Au[/mml mi][/mml mrow][/mml math] collisions at [mml math altimg="si2.gif" overflow="scroll" xmlns xocs="http //www.elsevier.com/xml/xocs/dtd" xmlns xs="http //www.w3.org/2001/XMLSchema" xmlns xsi="http //www.w3.org/2001/XMLSchema-instance" xmlns="http //www.elsevier.com/xml/ja/dtd" xmlns ja="http //www.elsevier.com/xml/ja/dtd" xmlns mml="http //www.w3.org/1998/Math/MathML" xmlns tb="http //www.elsevier.com/xml/common/table/dtd" xmlns sb="http //www.elsevier.com/xml/common/struct-bib/dtd" xmlns ce="http //www.elsevier.com/xml/common/dtd" xmlns xlink="http //www.w3.org/1999/xlink" xmlns cals="http //www.elsevier.com/xml/common/cals/dtd" xmlns sa="http //www.elsevier.com/xml/common/struct-aff/dtd"][mml msqrt][mml msub][mml mrow][mml mi][/mml mi][/mml mrow][mml mrow][mml mi mathvariant="normal"]NN[/mml mi][/mml mrow][/mml msub][/mml msqrt][mml mo]=[/mml mo][mml mn]200[/mml mn][mml mtext] [/mml mtext][mml mtext]GeV[/mml mtext][/mml math]( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

In this study, dihadron correlations are analyzed in √sNN = 200 GeV d+Au collisions classified by forward charged particle multiplicity and zero-degree neutral energy in the Au-beam direction. It is found that the jetlike correlated yield increases with the event multiplicity. After taking into account this dependence, the non-jet contribution on the away side is minimal, leaving little room for a back-to-back ridge in these collisions
The LMC geometry and outer stellar populations from early DES data( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

Cosmological implications of baryon acoustic oscillation measurements( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

Here, we derive constraints on cosmological parameters and tests of dark energy models from the combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave background (CMB) data and a recent reanalysis of Type Ia supernova (SN) data. In particular, we take advantage of high-precision BAO measurements from galaxy clustering and the Lyman-[alpha] forest (LyaF) in the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Treating the BAO scale as an uncalibrated standard ruler, BAO data alone yield a high confidence detection of dark energy; in combination with the CMB angular acoustic scale they further imply a nearly flat universe. Adding the CMB-calibrated physical scale of the sound horizon, the combination of BAO and SN data into an "inverse distance ladder" yields a measurement of H0=67.3±1.1 km s1 Mpc₋1, with 1.7% precision. This measurement assumes standard prerecombination physics but is insensitive to assumptions about dark energy or space curvature, so agreement with CMB-based estimates that assume a flat [Lambda]CDM cosmology is an important corroboration of this minimal cosmological model. For constant dark energy ([Lambda]), our BAO+SN+CMB combination yields matter density [Omega]m=0.301±0.008 and curvature [Omega]k=₋0.003±0.003. When we allow more general forms of evolving dark energy, the BAO+SN+CMB parameter constraints are always consistent with flat [Lambda]CDM values at H"[sigma]. While the overall [chi]2 of model fits is satisfactory, the LyaF BAO measurements are in moderate (2-2.5[sigma]) tension with model predictions. Models with early dark energy that tracks the dominant energy component at high redshift remain consistent with our expansion history constraints, and they yield a higher H0 and lower matter clustering amplitude, improving agreement with some low redshift observations. Expansion history alone yields an upper limit on the summed mass of neutrino species, [Sigma]m[nu]<0.56 eV (95% confidence), improving to [Sigma]m[nu]<0.25 eV if we include the lensing signal in the Planck CMB power spectrum. In a flat [Lambda]CDM model that allows extra relativistic species, our data combination yields Neff=3.43±0.26; while the LyaF BAO data prefer higher Neff when excluding galaxy BAO, the galaxy BAO alone favor Neff H"3. Lastly, when structure growth is extrapolated forward from the CMB to low redshift, standard dark energy models constrained by our data predict a level of matter clustering that is high compared to most, but not all, observational estimates
DES13S2cmm : the first superluminous supernova from the Dark Energy Survey( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

Simulation of transverse modes with their intrinsic Landau damping for bunched beams in the presence of space charge( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

Isolation of flow and nonflow correlations by two- and four-particle cumulant measurements of azimuthal harmonics in [arrow]"NN = 200 GeV Au+Au collisions( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

A data-driven method was applied to Au+Au collisions at [arrow]"NN = 200 GeV made with the STAR detector at RHIC to isolate pseudorapidity distance [Delta][eta]-dependent and [Delta][eta]-independent correlations by using two- and four-particle azimuthal cumulant measurements. We identified a [Delta][eta]-independent component of the correlation, which is dominated by anisotropic flow and flow fluctuations. It was also found to be independent of [eta] within the measured range of pseudorapidity
Measurements of the Upsilon(1S), Upsilon(2S), and Upsilon(3S) differential cross sections in pp collisions at sqrt(s) = 7 TeV( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

Differential cross sections as a function of transverse momentum pt are presented for the production of Y(nS) (n = 1, 2, 3) states decaying into a pair of muons. Data corresponding to an integrated luminosity of 4.9 inverse femtobarns in pp collisions at sqrt(s) = 7 TeV were collected with the CMS detector at the LHC. The analysis selects events with dimuon rapidity abs(y) <1.2 and dimuon transverse momentum in the range 10 <pt <100 GeV. The measurements show a transition from an exponential to a power-law behavior at pt ~ 20 GeV for the three Y states. Above that transition, the Y spectrum is significantly harder than that of the Y(1S) and Y(2S). The ratios of the Y(3S) and Y(2S) differential cross sections to the Y(1S) cross section show a rise as pt increases at low pt, then become flatter at higher pt
An ultra-weak sector, the strong CP problem and the pseudo-Goldstone dilaton( )

2 editions published between 2014 and 2015 in English and held by 0 WorldCat member libraries worldwide

In the context of a Coleman-Weinberg mechanism for the Higgs boson mass, we address the strong CP problem. We show that a DFSZ-like invisible axion model with a gauge-singlet complex scalar field S, whose couplings to the Standard Model are naturally ultra-weak, can solve the strong CP problem and simultaneously generate acceptable electroweak symmetry breaking. The ultra-weak couplings of the singlet S are associated with underlying approximate shift symmetries that act as custodial symmetries and maintain technical naturalness. The model also contains a very light pseudo-Goldstone dilaton that is consistent with cosmological Polonyi bounds, and the axion can be the dark matter of the universe. We further outline how a SUSY version of this model, which may be required in the context of Grand Unification, can avoid introducing a hierarchy problem
Search for Diphoton Resonances in the Mass Range from 150 to 850 GeV in pp Collisions at $\sqrt{s}$ = 8 TeV( )

10 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

Two searches for physics beyond the standard model in events containing photons are presented. Our data sample used corresponds to an integrated luminosity of 19.7 fb-1 of proton-proton collisions at √s=8 TeV, collected with the CMS experiment at the CERN LHC. The analyses pursue different inclusive search strategies. One analysis requires at least one photon, at least two jets, and a large amount of transverse momentum imbalance, while the other selects events with at least two photons and at least one jet, and uses the razor variables to search for signal events. The background expected from standard model processes is evaluated mainly from data. These results are interpreted in the context of general gauge-mediated supersymmetry, with the next-to-lightest supersymmetric particle either a bino- or wino-like neutralino, and within simplified model scenarios. Upper limits at the 95% confidence level are obtained for cross sections as functions of the masses of the intermediate supersymmetric particles
Searches for third-generation squark production in fully hadronic final states in proton-proton collisions at [arrow]" = 8 TeV( )

4 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

The purely electroweak (EW) cross section for the production of two jets in association with a Z boson, in proton-proton collisions at [arrow]" = 8 TeV, is measured using data recorded by the CMS experiment at the CERN LHC, corresponding to an integrated luminosity of 19.7 fb-1. The electroweak cross section for the lljj final state (with l = e or [mu] and j representing the quarks produced in the hard interaction) in the kinematic region defined by Mll> 50 GeV, Mjj> 120 GeV, transverse momentum pTj> 25 GeV, and pseudorapidity
First measurement of neutrino and antineutrino coherent charged pion production on argon( )

2 editions published between 2014 and 2015 in English and held by 0 WorldCat member libraries worldwide

We report on the first cross section measurements for charged current coherent pion production by neutrinos and antineutrinos on argon. These measurements are performed using the ArgoNeuT detector exposed to the NuMI beam at Fermilab. The cross sections are measured to be 2.6 +1.2-1.0 (stat)+0.3-0.4(syst) × 10⁻³⁸cm² / Ar for neutrinos at a mean energy of 9.6 GeV and 5.5+2.6-2.1(stat)+0.6-0.7(syst) × 10⁻³⁹ cm² / Ar for antineutrinos at a mean energy of 3.6 GeV
Search for W' decaying to tau lepton and neutrino in proton-proton collisions at $\sqrt{s}$ = 8 TeV( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

Results are reported of a general search for pair production of heavy resonances decaying to pairs of jets in events with at least four jets. The study is based on up to 19.4 inverse femtobarns of integrated luminosity from proton-proton collisions at a center-of-mass energy of 8 TeV, recorded with the CMS detector at the LHC. Limits are determined on the production of scalar top quarks (top squarks) in the framework of R-parity violating supersymmetry and on the production of color-octet vector bosons (colorons). First limits at the LHC are placed on top squark production for two scenarios. The first assumes decay to a bottom quark and a light-flavor quark and is excluded for masses between 200 and 385 GeV, and the second assumes decay to a pair of light-flavor quarks and is excluded for masses between 200 and 350 GeV at 95% confidence level. Previous limits on colorons decaying to light-flavor quarks are extended to exclude masses from 200 to 835 GeV
Final report by Yale University( )

5 editions published between 2012 and 2014 in English and held by 0 WorldCat member libraries worldwide

The activity reported includes work on several experiments (BNL E871 at Brookhaven National Lab, HERA-B at DESY, MINOS at Fermilab, BABAR at SLAC, and Minerva at Fermilab) and theory
MINERvA neutrino detector response measured with test beam data( )

2 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

The MINERvA collaboration operated a scaled-down replica of thesolid scintillator tracking and sampling calorimeter regions of the MINERvA detector in a hadron test beam at the Fermilab Test Beam Facility. This paper reports measurements with samples of protons, pions, and electrons from 0.35 to 2.0 GeV/c momentum. The calorimetric response to protons, pions, and electrons is obtained from these data. A measurement of the parameter in Birks' law and an estimate of the tracking efficiency are extracted from the proton sample. Overall the data are well described by a Geant4-based Monte Carlo simulation of the detector and particle interactions with agreements better than 4% for the calorimetric response, though some features of the data are not precisely modeled. These measurements are used to tune the MINERvA detector simulation and evaluate systematic uncertainties in support of the MINERvA neutrino cross-section measurement program
15 - Foot Bubble Chamber : Safety Report - Volume 1( )

2 editions published in 1972 in English and held by 0 WorldCat member libraries worldwide

Measurement of the ratio of the production cross sections times branching fractions of Bc" ₂!J/[psi][pi]"and B" ₂!J/[psi] K" and B(Bc"₂!J/[psi] [pi]"[pi]"[pi]-/+)/B(Bc" ₂!J/[psi] [pi]") in pp collisions at [arrow]" = 7 TeV( )

2 editions published between 2014 and 2015 in English and held by 0 WorldCat member libraries worldwide

The ratio of the production cross sections times branching fractions ([sigma](Bc") B(Bc" ₂!J/[psi][pi]"))/([sigma](B") B(B" ₂!J/[psi]K") is studied in proton-proton collisions at a center-of-mass energy of 7 TeV with the CMS detector at the LHC. The kinematic region investigated requires Ba, sub>c" and B"mesons with transverse momentum p[tau]> 15 GeV and rapidity
Search for Resonant $\mathrm{t\bar{t}}$ Production in Proton-Proton Collisions at $\sqrt{s}$ = 8 TeV( )

3 editions published in 2015 in English and held by 0 WorldCat member libraries worldwide

A search for new physics in proton-proton collisions having final states with an electron or muon and missing transverse energy is presented. The analysis uses data collected in 2012 with the CMS detector, at an LHC center-of-mass energy of 8 TeV, and corresponding to an integrated luminosity of 19.7 fb$^{-1}$. No significant deviation of the transverse mass distribution of the charged lepton-neutrino system from the standard model prediction is found. Mass exclusion limits of up to 3.28 TeV at a 95% confidence level for a W$^{\prime}$ boson with the same couplings as that of the standard model W boson are determined. Results are also derived in the framework of split universal extra dimensions, and exclusion limits on Kaluza-Klein W$^{(2)}_{{\rm KK}}$ states are found. The final state with large missing transverse energy also enables a search for dark matter production with a recoiling W boson, with limits set on the mass and the production cross section of potential candidates. Finally, limits are established for a model including interference between a left-handed W$^{\prime}$ boson and the standard model W boson, and for a compositeness model

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United States. Department of Energy. Office of Science. High Energy Physics Division

United States. Dept. of Energy. High Energy Physics Division

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English (54)