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  1. 5721
    por Nassibian, G
    Publicado 1986
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    The real part of the low frequency beam impedance of travelling wave kickers with arbitrary terminations
  2. 5722
    por Nassibian, G
    Publicado 1986
    Enlace del recurso
    The real part of the low frequency beam impedance of travelling wave kickers with arbitrary terminations
  3. 5723
    “…Several linacs comprise different traveling-wave (TW) accelerating structures fulfilling the beam dynamics and rf constraints. …”
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    RF Design of Traveling-Wave Accelerating Structures for the FCC-ee Pre-injector Complex
  4. 5724
    por Pearce, P
    Publicado 1994
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    Technical specification for the purchase of a 30 GHz travelling wave tube amplifier system
  5. 5725
    “…We explore the impact of choosing different sets of time-delay interferometry (TDI) variables for detecting and reconstructing stochastic gravitational wave background (SGWB) signals and estimating the instrumental noise in LISA. …”
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    Stochastic gravitational wave background reconstruction for a nonequilateral and unequal-noise LISA constellation
  6. 5726
    “…We use the latest constraints on the population of stellar origin binary black holes (SOBBH) from LIGO/Virgo/KAGRA (LVK) observations, to estimate the stochastic gravitational wave background (SGWB) they generate in the frequency band of LISA.In order to account for the faint and distant binaries, which contribute the most to the SGWB, we extend the merger rate at high redshift assuming that it tracks the star formation rate.We adopt different methods to compute the SGWB signal: we perform an analytical evaluation, we use Monte Carlo sums over the SOBBH population realisations, and we account for the role of the detector by simulating LISA data and iteratively removing the resolvable signals until only the confusion noise is left.The last method allows the extraction of both the expected SGWB and the number of resolvable SOBBHs.Since the latter are few for signal-to-noise ratio thresholds larger than five, we confirm that the spectral shape of the SGWB in the LISA band agrees with the analytical prediction of a single power law.We infer the probability distribution of the SGWB amplitude from the LVK GWTC-3 posterior of the binary population model: at the reference frequency of 0.003 Hz it has an interquartile range of h$^{2}$Ω$_{GW}$(f = 3 × 10$^{-3}$ Hz) ∈ [5.65, 11.5] × 10$^{-13}$, in agreement with most previous estimates.We then perform a MC analysis to assess LISA's capability to detect and characterise this signal.Accounting for both the instrumental noise and the galactic binaries foreground, with four years of data, LISA will be able to detect the SOBBH SGWB with percent accuracy,narrowing down the uncertainty on the amplitude by one order of magnitude with respect to the range of possible amplitudes inferred from the population model. …”
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    Stochastic gravitational wave background from stellar origin binary black holes in LISA
  7. 5727
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    The N-soliton dynamics of the shallow water wave equation and the Korteweg-de Vries hierarchy
  8. 5728
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    Tuning of 5.2 metre long tapered S-band traveling wave accelerating section
  9. 5729
    por Albrecht, H, Hamacher, T, Hofmann, R P, Kirchhoff, T, Mankel, R, Nau, A, Nowak, S, Ressing, D, Schröder, H, Schulz, H D, Walter, M, Wurth, R, Hast, C, Kapitza, H, Kolanoski, H, Kosche, A, Lange, A, Lindner, A, Schieber, M, Siegmund, T, Thurn, H, Töpfer, D, Wegener, D, Frankl, C, Graf, J, Schmidtler, M, Schramm, M, Schubert, Klaus R, Schwierz, R, Spaan, B, Waldi, R, Reim, K, Wegener, H, Eckmann, R, Kuipers, H, Mai, O, Mundt, R, Oest, T, Reiner, R, Schmidt-Parzefall, W, Stiewe, J, Werner, S, Ehret, K, Hofmann, W, Hüpper, A, Knöpfle, K T, Spengler, J, Krieger, P, MacFarlane, D B, Prentice, J D, Saull, P R B, Tzamariudaki, K, van de Water, R, Yoon, T S, Schneider, M, Weseler, S, Bracko, M, Kernel, G, Krizan, P, Kriznic, E, Medin, G, Podobnik, T, Zivko, T, Balagura, V, Barsuk, S, Belyaev, I, Chistov, R, Danilov, M V, Eiges, V, Gershtein, L I, Gershtein, Yu, Golutvin, A, Igonkina, O, Korolko, I, Kostina, G, Litvintsev, D O, Pakhlov, P, Semenov, S V, Snizhko, A, Tichomirov, I, Zaitsev, Yu
    Publicado 1996
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    A partial wave analysis of the reaction $\gamma\gamma$ --> $\pi^{+}$ $\pi^{-}\pi^{0}$
  10. 5730
    por Ackerstaff, K, Alexander, Gideon, Allison, J, Altekamp, N, Anderson, K J, Anderson, S, Arcelli, S, Asai, S, Axen, D A, Azuelos, Georges, Ball, A H, Barberio, E, Barlow, R J, Bartoldus, R, Batley, J Richard, Baumann, S, Bechtluft, J, Beeston, C, Behnke, T, Bell, A N, Bell, K W, Bella, G, Bentvelsen, Stanislaus Cornelius Maria, Berlich, P, Bethke, Siegfried, Biebel, O, Biguzzi, A, Bird, S D, Blobel, Volker, Bloodworth, Ian J, Bloomer, J E, Bobinski, M, Bock, P, Bonacorsi, D, Boutemeur, M, Bouwens, B T, Braibant, S, Brigliadori, L, Brown, R M, Burckhart, Helfried J, Burgard, C, Bürgin, R, Capiluppi, P, Carnegie, R K, Carter, A A, Carter, J R, Chang, C Y, Charlton, D G, Chrisman, D, Clarke, P E L, Cohen, I, Conboy, J E, Cooke, O C, Cuffiani, M, Dado, S, Dallapiccola, C, Dallavalle, G M, De Jong, S, del Pozo, L A, Desch, Klaus, Dixit, M S, do Couto e Silva, E, Doucet, M, Duchovni, E, Duckeck, G, Duerdoth, I P, Eatough, D, Edwards, J E G, Estabrooks, P G, Evans, H G, Evans, M, Fabbri, Franco Luigi, Fanti, M, Faust, A A, Fiedler, F, Fierro, M, Fischer, H M, Fleck, I, Folman, R, Fong, D G, Foucher, M, Fürtjes, A, Futyan, D I, Gagnon, P, Gary, J W, Gascon, J, Gascon-Shotkin, S M, Geddes, N I, Geich-Gimbel, C, Geralis, T, Giacomelli, G, Giacomelli, P, Giacomelli, R, Gibson, V, Gibson, W R, Gingrich, D M, Glenzinski, D A, Goldberg, J, Goodrick, M J, Gorn, W, Grandi, C, Gross, E, Grunhaus, Jacob, Gruwé, M, Hajdu, C, Hanson, G G, Hansroul, M, Hapke, M, Hargrove, C K, Hart, P A, Hartmann, C, Hauschild, M, Hawkes, C M, Hawkings, R, Hemingway, Richard J, Herndon, M, Herten, G, Heuer, R D, Hildreth, M D, Hill, J C, Hillier, S J, Hilse, T, Hobson, P R, Homer, R James, Honma, A K, Horváth, D, Howard, R, Hutchcroft, D E, Igo-Kemenes, P, Imrie, D C, Ingram, M R, Ishii, K, Jawahery, A, Jeffreys, P W, Jeremie, H, Jimack, Martin Paul, Joly, A, Jones, C R, Jones, G, Jones, M, Jost, U, Jovanovic, P, Junk, T R, Karlen, D A, Kartvelishvili, V G, Kawagoe, K, Kawamoto, T, Keeler, Richard K, Kellogg, R G, Kennedy, B W, Kirk, J, Klier, A, Kluth, S, Kobayashi, T, Kobel, M, Koetke, D S, Kokott, T P, Kolrep, M, Komamiya, S, Kress, T, Krieger, P, Von Krogh, J, Kyberd, P, Lafferty, G D, Lahmann, R, Lai, W P, Lanske, D, Lauber, J, Lautenschlager, S R, Layter, J G, Lazic, D, Lee, A M, Lefebvre, E, Lellouch, Daniel, Letts, J, Levinson, L, Lloyd, S L, Loebinger, F K, Long, G D, Losty, Michael J, Ludwig, J, Macchiolo, A, MacPherson, A L, Mannelli, M, Marcellini, S, Markus, C, Martin, A J, Martin, J P, Martínez, G, Mashimo, T, Mättig, P, McDonald, W J, McKenna, J A, McKigney, E A, McMahon, T J, McPherson, R A, Meijers, F, Menke, S, Merritt, F S, Mes, H, Meyer, J, Michelini, Aldo, Mikenberg, G, Miller, D J, Mincer, A, Mir, R, Mohr, W, Montanari, A, Mori, T, Morii, M, Müller, U, Nagai, K, Nakamura, I, Neal, H A, Nellen, B, Nisius, R, O'Neale, S W, Oakham, F G, Odorici, F, Ögren, H O, Oldershaw, N J, Oreglia, M J, Orito, S, Pálinkás, J, Pásztor, G, Pater, J R, Patrick, G N, Patt, J, Pearce, M J, Petzold, S, Pfeifenschneider, P, Pilcher, J E, Pinfold, James L, Plane, D E, Poffenberger, P R, Poli, B, Posthaus, A, Przysiezniak, H, Rees, D L, Rigby, D, Robertson, S, Robins, S A, Rodning, N L, Roney, J M, Rooke, A M, Ros, E, Rossi, A M, Rosvick, M, Routenburg, P, Rozen, Y, Runge, K, Runólfsson, O, Ruppel, U, Rust, D R, Rylko, R, Sachs, K, Saeki, T, Sarkisyan-Grinbaum, E, Sbarra, C, Schaile, A D, Schaile, O, Scharf, F, Scharff-Hansen, P, Schenk, P, Schieck, J, Schleper, P, Schmitt, B, Schmitt, S, Schöning, A, Schröder, M, Schultz-Coulon, H C, Schulz, M, Schumacher, M, Schwick, C, Scott, W G, Shears, T G, Shen, B C, Shepherd-Themistocleous, C H, Sherwood, P, Siroli, G P, Sittler, A, Skillman, A, Skuja, A, Smith, A M, Snow, G A, Sobie, Randall J, Söldner-Rembold, S, Springer, R W, Sproston, M, Stephens, K, Steuerer, J, Stockhausen, B, Stoll, K, Strom, D, Szymanski, P, Tafirout, R, Talbot, S D, Tanaka, S, Taras, P, Tarem, S, Teuscher, R, Thiergen, M, Thomson, M A, Von Törne, E, Towers, S, Trigger, I, Tsur, E, Turcot, A S, Turner-Watson, M F, Utzat, P, Van Kooten, R, Verzocchi, M, Vikas, P, Vokurka, E H, Voss, H, Wäckerle, F, Wagner, A, Ward, C P, Ward, D R, Watkins, P M, Watson, A T, Watson, N K, Wells, P S, Wermes, N, White, J S, Wilkens, B, Wilson, G W, Wilson, J A, Wolf, G, Wyatt, T R, Yamashita, S, Yekutieli, G, Zacek, V, Zer-Zion, D
    Publicado 1997
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    Production of P-wave charm and charm-strange mesons in hadronic $Z^0$ decays
  11. 5731
    por Anderson, D E, Stover, G D
    Publicado 1998
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    Design of quasi-traveling wave pinger magnet for beam diagnostics on the Advanced Light Source
  12. 5732
    Enlace del recurso
    RF measurements of a traveling-wave muffin-tin accelerating structure at 90 GHz
  13. 5733
    por Costa de Lima, M, Damião-Soares, I
    Publicado 1997
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    Gravitational wave emission and mass extraction from a perturbed Schwarzschild black hole
  14. 5734
    Enlace del recurso
    Design and fabrication of a traveling-wave muffin-tin accelerating structure at 90 GHz
  15. 5735
    Enlace del recurso
    Outsourcing of the New Wave Form Acquisition, Surveillance and Diagnostic System for the LEP Injection Kickers
  16. 5736
    Enlace del recurso
    Upper limit for a gravitational-wave stochastic background with the EXPLORER and NAUTILUS resonant detectors
  17. 5737
    Enlace del recurso
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    A simple derivation of the normalization condition for the bound-state Bethe-Salpeter wave function
  18. 5738
    Enlace del recurso
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    (p,2p) reactions at 600 MeV and the distorted-wave impulse approximation
  19. 5739
    por Alam, S, Bentley, C
    Publicado 1998
    Enlace del recurso
    Nonlinear model for trapped ion interacting with standing wave via gauge-like transformations
  20. 5740
    “…A Study of Charged P-wave D Meson Production in Semileptonic B Decays. …”
    Enlace del recurso
    A Study of Charged P-wave D Meson Production in Semileptonic B Decays
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