Physics Commons^™

A Sub-Kpc-Scale Binary Active Galactic Nucleus With Double Narrow-Line Regions, Jong-Hak Woo, Hojin Cho, Bernd Husemann, S. Komossa, Daeseong Park, Vardha N. Bennert

Physics

We present the kinematic properties of a type-2 Quasi stellar object (QSO), SDSS J132323.33−015941.9 at z ∼ 0.35, based on the analysis of Very Large Telescope integral field spectroscopy and Hubble Space Telescope (HST) imaging, which suggest that the target is a binary active galactic nucleus (AGN) with double narrow-line regions. The QSO features double-peaked emission lines ([O iii] and Hβ) which can be decomposed into two kinematic components. The flux-weighted centroids of the blue and red components are separated by ∼0.2 arcsec (0.8 kpc in projection) and coincide with the location of the two stellar cores detected …

Longitudinal Emittance Blowup In The Large Hadron Collider, P. Baudrenghien, T. Mastoridis

Physics

The Large Hadron Collider (LHC) relies on Landau damping for longitudinal stability. To avoid decreasing the stability margin at high energy, the longitudinal emittance must be continuously increased during the acceleration ramp. Longitudinal blowup provides the required emittance growth. The method was implemented through the summer of 2010. Band-limited RF phase-noise is injected in the main accelerating cavities during the whole ramp of about 11 min. Synchrotron frequencies change along the energy ramp, but the digitally created noise tracks the frequency change. The position of the noise-band, relative to the nominal synchrotron frequency, and the bandwidth of the spectrum are …

Bayesian Approach For Uncertainty Analysis Of An Urban Storm Water Model And Its Applications To A Heavily Urbanized Watershed, Misgana K. Muleta, Jonathan Mcmillan, Geremew G. Amenu, Steven J. Burian

Physics

The significance of uncertainty analysis (UA) to quantify reliability of model simulations is being recognized. Consequently, literature on parameter and predictive uncertainty assessment of water resources models has been rising. Applications dealing with urban drainage systems are, however, very limited. This study applies formal Bayesian approach for uncertainty analysis of a widely used storm water management model and illustrates the methodology using a highly urbanized watershed in the Los Angeles Basin, California. A flexible likelihood function that accommodates heteroscedasticity, non-normality, and temporal correlation of model residuals has been used for the study along with a Markov-chain Monte Carlo-based sampling scheme. …

Discovery Of An Eo-Meso-Neoarchean Terrane In The East Greenland Caledonides, Scott M. Johnston, Andrew R.C. Kylander-Clark

Physics

tThis study investigates basement gneisses from the Niggli Spids thrust sheet of the East Greenland Caledonides in an attempt to place them into the broader context of the Archean–Paleoproterozoicarchitecture of the Greenland shield. Our combined whole-rock geochemical and U–Pb zircon geochronol-ogy results from Gåseland reveal an Archean terrane defined by TTG magmatic events at 3607 Ma and3070–2980 Ma followed by metamorphism and high-K granite intrusion at 2790–2677 Ma. These results identify a relatively pristine Archean terrane with previously unknown Eoarchean rocks that holds poten-tial for future investigations into the early evolution of continental crust, and adds to a growing body …

The Lick Agn Monitoring Project 2011: Fe Ii Reverberation From The Outer Broad-Line Region, Aaron J. Barth, Anna Pancoast, Vardha N. Bennert, Brendon J. Brewer, Gabriela Canalizo, Alexei V. Filippenko, Elinor L. Gates, Jenny E. Greene, Weidong Li, Matthew A. Malkan, David J. Sand, Daniel Stern, Tommaso Treu, Jong-Hak Woo, Roberto J. Assef, Hyun-Jin Bae, Tabitha Buehler, S. Bradley Cenko, Kelsey I. Clubb, Michael C. Cooper, Aleksander M. Diamond-Stanic, Sebastian F. Hönig, Michael D. Joner, C. David Laney, Mariana S. Lazarova, A. M. Nierenberg, Jeffrey M. Silverman, Erik J. Tollerud, Jonelle L. Walsh

Physics

The prominent broad Fe ii emission blends in the spectra of active galactic nuclei have been shown to vary in response to continuum variations, but past attempts to measure the reverberation lag time of the optical Fe ii lines have met with only limited success. Here we report the detection of Fe ii reverberation in two Seyfert 1 galaxies, NGC 4593 and Mrk 1511, based on data from a program carried out at Lick Observatory in Spring 2011. Light curves for emission lines including Hβ and Fe ii were measured by applying a fitting routine to decompose the spectra into …

Update On Beam Induced Rf Heating In The Lhc, B. Salvant, O. Aberle, G. Arduini, R. Assmann, B. Baglin, M.J. Barnes, W. Bartmann, P. Baudrenghien, O. Berrig, C. Bracco, E. Bravin, G. Bregliozzi, R. Bruce, A. Bertarelli, F. Carra, G. Cattenoz, F. Caspers, S. Claudet, H. Day, M. Garlasche, L. Gentini, B. Goddard, A. Grudiev, B. Henrist, R. Jones, O. Kononenko, G. Lanza, L. Lari, T. Mastoridis, V. Mertens, E. Métral, N. Mounet, J.E. Muller, A.A. Nosych, J.L. Nougaret, S. Persichelli, A.M. Piguiet, S. Redaelli, F. Roncarolo, G. Rumolo, B. Salvachua, M. Sapinski, R. Schmidt, E. Shaposhnikova, L. Tavian, M. Timmins, J. Uythoven, A. Vidal, J. Wenninger, D. Wollmann, M. Zerlauth, P. Fassnacht, S. Jakobsen, M. Deile

Physics

Since June 2011 the rapid increase of the luminosity performance of the LHC has come at the expense of both increased temperature and pressure of specific, near-beam, LHC equipment. In some cases, this beam induced heating has caused delays while equipment cool-down, beam dumps and even degradation of some devices. This contribution gathers the observations of beam induced heating, attributed to longitudinal beam coupling impedance, their current level of understanding and possible actions planned to be implemented during the 1st LHC Long Shutdown (LS1) in 2013-2014.

Investigations Of The Lhc Emittance Blow-Up During The 2012 Proton Run, M. Kuhn, G. Arduini, P. Baudrenghien, J. Emery, A. Guerrero, W. Hofle, V. Kain, M. Lamont, T. Mastoridis, F. Roncarolo, M. Sapinski, M. Schaumann, R. Steinhagen, G. Trad, D. Valuch

Physics

About 30 % of the potential luminosity performance is lost through the different phases of the LHC cycle, mainly due to transverse emittance blow-up. Measuring the emittance growth is a difficult task with high intensity beams and changing energies. Improvements of the LHC transverse profile instrumentation helped to study various effects. A breakdown of the growth through the different phases of the LHC cycle is given as well as a comparison with the data from the LHC experiments for transverse beam size. In 2012 a number of possible sources and remedies have been studied. Among these are intra beam scattering, …

Search For 14.4 Kev Solar Axions From M1 Transition Of 57fe With Cuore Crystals, F. Alessandria, R Ardito, D. R. Artusa, F.T. Avignone Iii, O. Azzolini, M Balata, T.I. Banks, G. Bari, J. Beeman, F Bellini, A. Bersani, M. Biassoni, T. Bloxham, C Brofferio, C Bucci, X.Z. Cai, L. Canonica, S Capelli, L. Carbone, L. Cardani, M. Carrettoni, N. Casali, N. Chott, M Clemenza, C Cosmelli, O Cremonesi, R.J. Creswick, I Dafinei, A. Dally, V. Datskov, A. De Biasi, M.P. Decowski, M. M. Deninno, S Di Domizio, M.L. Di Vacri, L. Ejzak, R. Faccini, D.Q. Fang, H.A. Farach, E. Ferri, F Ferroni, E Fiorini, M.A. Franceschi, S.J. Freedman, B.K. Fujikawa, A Giachero, L. Gironi, A Giuliani, J. Goett, P Gorla, C. Gotti, E Guardincerri, T. D. Gutierrez, E.E. Haller, K. Han, K.M. Heeger, H.Z. Huang, R. Kadel, G. Keppel, L. Kogler, Yu. G. Kolomensky, D. Lenz, Y.L. Li, C. Ligi, X. Liu, Y.G. Ma, C. Maiano, M. Maino, M. Martinez, R.H. Maruyama, N. Moggi, S Morganti, T. Napolitano, S. Newman, S Nisi, C Nones, E.B. Norman, A Nucciotti, F. Orio, D. Orlandi, J.L. Ouellet, M Pallavicini, E. Palmieri, L. Pattavina, M Pavan, M Pedretti, G Pessina, S Pirro, E Previtali, V. Rampazzo, F. Rimondi, C Rosenfeld, C. Rusconi, S Sangiorgio, N.D. Scielzo, M Sisti, A.R. Smith, L. Taffarello, M. Tenconi, W.D. Tian, C. Tomei, S. Trentalange, G Ventura, M Vignati, B.S. Wang, H.W. Wang, C. A. Whitten Jr., T. Wise, A. Woodcraft, L Zanotti, C. Zarra, B.X. Zhu, S. Zucchelli

Physics

We report the results of a search for axions from the 14.4 keV M1 transition from ⁵⁷Fe in the core of the sun using the axio-electric effect in TeO₂bolometers. The detectors are 5

× 5 × 5 cm³ crystals operated at about 10 mK in a facility used to test bolometers for the CUORE experiment at the Laboratori Nazionali del Gran Sasso in Italy. An analysis of 43.65 kg⋅d of data was made using a newly developed low energy trigger which was optimized to reduce the energy threshold of the detector. An upper limit of 0.58 …

Validation Of Techniques To Mitigate Copper Surface Contamination In Cuore, F. Alessandria, R. Ardito, D.R. Artusa, F.T. Avignone Iii, O. Azzolini, M. Balata, T.I. Banks, G. Bari, J. Beeman, F. Bellini, A. Bersani, M. Biassoni, T. Bloxham, C. Brofferio, C. Bucci, X.Z. Cai, L. Canonica, S. Capelli, L. Carbone, L. Cardani, M. Carrettoni, N. Casali, N. Chott, M. Clemenza, C. Cosmelli, O. Cremonesi, R.J. Creswich, I. Dafinei, A. Dally, V. Datskov, A. De Biasi, M.M. Deninno, S. Di Domizio, M.L. Di Vacri, L. Ejzak, R. Faccini, D.Q. Fang, H.A. Farach, E. Ferri, F. Ferroni, E. Fiorini, M.A. Franceschi, S.J. Freedman, B.K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, J. Goett, A. Goodsell, P. Gorla, C. Gotti, E. Guardincerri, T.D. Gutierrez, E.E. Haller, K. Han, K.M. Heeger, H.Z. Huang, R. Kadel, K. Kazkaz, G. Keppel, L. Kogler, Yu. G. Kolomensky, D. Lenz, Y.L. Li, C. Ligi, X. Liu, Y.G. Ma, C. Maiano, M. Maino, M. Martinez, R.H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, S. Newman, S. Nisi, C. Nones, E.B. Norman, A. Nucciotti, F. Orio, D. Orlandi, J.L. Ouellet, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, M. Pedretti, G. Pessina, S. Pirro, E. Previtali, V. Rampazzo, R. Reil, F. Rimondi, C. Rosenfeld, C. Rusconi, S. Sangiorgio, N.D. Scielzo, M. Sisti, A.R. Smith, L. Sparks, F. Stivanello, L. Taffarello, M. Tenconi, W.D. Tian, C. Tomei, S. Trentalange, G. Ventura, M. Vignati, B.S. Wang, H.W. Wang, C.A. Whitten Jr, T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B.X. Zhu, S. Zucchelli

Physics

In this article we describe the background challenges for the CUORE experiment posed by surface contamination of inert detector materials such as copper, and present three techniques explored to mitigate these backgrounds. Using data from a dedicated test apparatus constructed to validate and compare these techniques we demonstrate that copper surface contamination levels better than 10⁻⁷- 10⁻⁸ Bq/cm² are achieved for ²³⁸U and ²³²Th. If these levels are reproduced in the final CUORE apparatus the projected 90% C.L. upper limit on the number of background counts in the region of interest is 0.02–0.03 counts/keV/kg/y …

The Extended Narrow-Line Region Of Two Type-I Quasi-Stellar Objects, Semyeong Oh, Jong-Hak Woo, Vardha N. Bennert, Bruno Jungwiert, Martin Haas, Christian Leipski, Marcus Albrecht

Physics

We investigate the narrow-line region (NLR) of two radio-quiet QSOs, PG1012+008 and PG1307+085, using high signal-to-noise spatially resolved long-slit spectra obtained with FORS1 at the Very Large Telescope. Although the emission is dominated by the point-spread function of the nuclear source, we are able to detect extended NLR emission out to several kiloparsec scales in both QSOs by subtracting the scaled central spectrum from outer spectra. In contrast to the nuclear spectrum, which shows a prominent blue wing and a broad line profile of the [Oiii] line, the extended emission reveals no clear signs of large-scale outflows. Exploiting the wide …

The Low-Luminosity End Of The Radius-Luminosity Relationship For Active Galactic Nuclei, Misty C. Bentz, Kelly D. Denney, Catherine J. Grier, Aaron J. Barth, Bradley M. Peterson, Marianne Vestergaard, Vardha N. Bennert, Gabriela Canalizo, Gisella De Rosa, Alexei V. Filippenko, Elinor L. Gates, Jenny E. Greene, Weidong Li, Matthew A. Malkan, Richard W. Pogge, Daniel Stern, Tommaso Treu, Jong-Hak Woo

Physics

We present an updated and revised analysis of the relationship between the Hβ broad-line region (BLR) radius and the luminosity of the active galactic nucleus (AGN). Specifically, we have carried out two-dimensional surface brightness decompositions of the host galaxies of nine new AGNs imaged with the Hubble Space Telescope Wide Field Camera 3. The surface brightness decompositions allow us to create “AGN-free” images of the galaxies, from which we measure the starlight contribution to the optical luminosity measured through the ground-based spectroscopic aperture. We also incorporate 20 new reverberation-mapping measurements of the Hβ time lag, which is assumed to yield …

Computational Problems In Introductory Physics: Lessons From A Bead On A Wire, Thomas J. Bensky, Matthew J. Moelter

Physics

We have found that incorporating computer programming into introductory physics requires problems suited for numerical treatment while still maintaining ties with the analytical themes in a typical introductory-level university physics course. In this paper, we discuss a numerical adaptation of a system commonly encountered in the introductory physics curriculum: the dynamics of an object constrained to move along a curved path. A numerical analysis of this problem that includes a computer animation can provide many insights and pedagogical avenues not possible with the usual analytical treatment. We present two approaches for computing the instantaneous kinematic variables of an object constrained …

The Low Energy Spectrum Of Teo2 Bolometers: Results And Dark Matter Perspectives For The Cuore-0 And Cuore Experiments, F. Alessandria, R. Ardito, D.R. Artusa, F.T. Avignone Iii, O. Azzolini, M. Balata, T.I. Banks, G. Bari, J. Beeman, F. Bellini, A. Bersani, M. Biassoni, T. Bloxham, C. Brofferio, C. Bucci, X.Z. Cai, L. Canonica, S. Capelli, L. Carbone, L. Cardani, M. Carrettoni, N. Casali, N. Chott, M. Clemenza, C. Cosmelli, O. Cremonesi, R.J. Creswick, I. Dafinei, A. Dally, V. Datskov, A. De Biasi, M.P. Decowski, M.M. Deninno, S. Di Domizio, M.L. Di Vacri, L. Ejzak, R. Faccini, D.Q. Fang, H.A. Farach, E. Ferri, F. Ferroni, E. Fiorini, M.A. Franceschi, S.J. Freedman, B.K. Fujikawa, A. Giachero, L. Gironi, A. Guiliani, J. Goett, P. Gorla, C. Gotti, E. Guardincerri, T.D. Gutierrez, E.E. Haller, K. Han, K.M. Heeger, H.Z. Huang, R. Kadel, K. Kazkaz, G. Keppel, L. Kogler, Yu. G. Kolomensky, D. Lenz, Y.L. Li, C. Ligi, X. Liu, Y.G. Ma, C. Maino, M. Maino, M. Martinez, R.H. Maruyama, N. Moggi, S. Morganti, T. Napolitano, S. Newman, S. Nisi, C. Nones, E.B. Norman, A. Nucciotti, F. Orio, D. Orlandi, J.L. Ouellet, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, M. Pedretti, G. Pessina, S. Pirro, E. Previtali, V. Rampazzo, F. Rimondi, C. Rosenfeld, C. Rusconi, S. Sangiorgio, N.D. Scielzo, M. Sisti, A.R. Smith, F. Stivanello, L. Taffarello, M. Tenconi, W.D. Tian, C. Tomei, S. Trentalange, G. Ventura, M. Vignati, B.S. Wang, H.W. Wang, C.A. Whitten Jr., T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B.X. Zhu, S. Zucchelli

Physics

We collected 19.4 days of data from four 750 g TeO2 bolometers, and in three of them we were able to set the energy threshold around 3 keV using a new analysis technique. We found a background rate ranging from 25 cpd/keV/kg at 3 keV to 2 cpd/keV/kg at 25 keV, and a peak at 4.7 keV. The origin of this peak is presently unknown, but its presence is confirmed by a reanalysis of 62.7 kg·days of data from the finished CUORICINO experiment. Finally, we report the expected sensitivities of the CUORE-0 (52 bolometers) and CUORE (988 bolometers) experiments to …

The Properties Of Post-Starburst Quasars Based On Optical Spectroscopy, Sabrina L. Cales, Michael S. Brotherton, Zhaohui Shang, Jessie C. Runnoe, Michael A. Dipompeo, Vardha Nicola Bennert, Gabriela Canalizo, Kyle D. Hiner, R. Stoll, Rajib Ganguly, Aleksandar Diamond-Stanic

Physics

We present optical spectroscopy of a sample of 38 post-starburst quasars (PSQs) at z ~ 0.3, 29 of which have morphological classifications based on Hubble Space Telescope imaging. These broad-lined active galactic nuclei (AGNs) possess the spectral signatures of massive intermediate-aged stellar populations, making them potentially useful for studying connections between nuclear activity and host galaxy evolution. We model the spectra in order to determine the ages and masses of the host stellar populations, and the black hole masses and Eddington fractions of the AGNs. Our model components include an instantaneous starburst, a power law, and emission lines. We find …