Search Results - "Fayer, S."

Towards an Improved Test of the Standard Model’s Most Precise Prediction by Gabrielse, G., Fayer, S., Myers, T., Fan, X.

“…The electron and positron magnetic moments are the most precise prediction of the standard model of particle physics. The most accurate measurement of a…”
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Positronium Production and Scattering below Its Breakup Threshold by Brawley, S J, Fayer, S E, Shipman, M, Laricchia, G

“…Recent findings on the similarity between electron and positronium scattering at the same velocity [Brawley et al., Science 330, 789 (2010)] have guided us…”
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Absolute Differential Positronium-Formation Cross Sections by Shipman, M, Armitage, S, Beale, J, Brawley, S J, Fayer, S E, Garner, A J, Leslie, D E, Van Reeth, P, Laricchia, G

“…The first absolute experimental determinations of the differential cross sections for the formation of ground-state positronium are presented for He, Ar, H2,…”
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A statistical description of scattering at the quantum level by Laricchia, G., Van Reeth, P., Fayer, S. E., Brawley, S. J., Kadokura, R., Loreti, A., Shipman, M.

“…Quantum physics is undoubtedly the most successful theory of the microscopic world, yet the complexities which arise in applying it even to simple atomic and…”
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Switchable Damping for a One-Particle Oscillator by Fan, X, Fayer, S. E, Myers, T. G, Sukra, B. A. D, Nahal, G, Gabrielse, G

“…Review of Scientific Instruments 92, 023201 (2021) The possibility to switch the damping rate for a one-electron oscillator is demonstrated, for an electron…”
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Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment by Alsum, S.K., Angelides, N., Araújo, H.M., Arthurs, M., Bai, X., Balajthy, J., Balashov, S., Baxter, A., Bernard, E.P., Birch, H.J., Boast, K.E., Boxer, B., Buckley, J.H., Bugaev, V.V., Busenitz, J.K., Cabrita, R., Carels, C., Carmona-Benitez, M.C., Cole, A., Cottle, A., Cutter, J.E., Viveiros, L. de, Druszkiewicz, E., Fan, A., Fayer, S., Fruth, T., Ghag, C., Gibson, E., Gokhale, S., van der Grinten, M.G.D., Harrison, A., Hertel, S.A., Hor, J.Y-K., Huang, D.Q., Ignarra, C.M., Ji, W., Kaboth, A.C., Kazkaz, K., Kocher, C.D., Korley, L., Korolkova, E.V., Kras, J., Kraus, H., Kravitz, S., Kudryavtsev, V.A., Leason, E.A., Lee, J., Lesko, K.T., Levy, C., Li, J., Liao, J., Liao, F.-T., Lin, J., Liu, R., Loniewski, C., Lopes, M.I., Lorenzon, W., Luitz, S., Manalaysay, A., Manenti, L., McLaughlin, J., Meng, Y., Miller, E.H., Mizrachi, E., Morad, J.A., Morrison, E., Nehrkorn, C., Nilima, A., Oliver-Mallory, K.C., Parveen, N., Piepke, A., Pushkin, K., Richards, A., Rutherford, G., Sazzad, A.B.M.R., Schnee, R.W., Seymour, D., Shaw, S., Silk, J.J., Smith, R., Stancu, I., Stevens, A., Stifter, K., Swanson, N., Tan, M., Taylor, R., Temples, D.J., Tiedt, D.R., Timalsina, M., Tripathi, M., Tvrznikova, L., Vaitkus, A., Wang, J.J., Wang, W., Webb, R.C., Whitis, T.J., Woodward, D., Xiang, X., Yeh, M., Zarzhitsky, P.

“…The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1–2)×10−12 pb at a WIMP mass of 40 …”
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High-Resolution Measurements of e super(+)+H sub(2) O Total Cross Section by Loreti, A, Kadokura, R, Fayer, S E, Kover, A, Laricchia, G

“…Using a purely electrostatic positron beam, the total cross section of positrons scattering from H sub(2) O has been measured for the first time with a high…”
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High-Resolution Measurements of e + + H 2 O Total Cross Section by Loreti, A., Kadokura, R., Fayer, S. E., Kövér, Á., Laricchia, G.

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Characterisation of the muon beams for the Muon Ionisation Cooling Experiment by Adams, D., Apollonio, M., Asfandiyarov, R., Back, J., Barber, G., Barclay, P., Bayes, R., Bertoni, R., Blackmore, V. J., Blondel, A., Blot, S., Bonesini, M., Booth, C. N., Boyd, S., Bradshaw, T. W., Bravar, U., Bross, A. D., Capponi, M., Cecchet, G., Colling, D., Collomb, N., Cremaldi, L. M., Dick, A. J., Fayer, S., Filthaut, F., Fish, A., Fletcher, R., Francis, V., Fry, L., Gallagher, A., Graulich, J. S., Griffiths, S., Hanlet, P., Hanson, G. G., Harrison, P., Hart, T. L., Hartnett, T., Hayler, T., Hodgson, P., Hunt, C., Iaciofano, A., Ishimoto, S., Kaplan, D. M., Karadzhov, Y., Kim, Y. K., Kolev, D., Kuno, Y., Kyberd, P., Lau, W., Leonova, M., Li, D., Lintern, A., Littlefield, M., Lucchini, G., Luo, T., Macwaters, C., Martlew, B., Middleton, S., Moretti, A., Moss, A., Muir, A., Mullacrane, I., Nebrensky, J. J., Nicholson, R., Onel, Y., Orestano, D., Owens, P., Palladino, V., Palmer, R. B., Pasternak, J., Pastore, F., Pidcott, C., Preece, R., Rajaram, D., Ramberger, S., Rayner, M. A., Ricciardi, S., Richards, A., Roberts, T. J., Robinson, M., Rogers, C., Ronald, K., Rubinov, P., Rusinov, I., Sanders, D. A., Santos, E., Smith, P. J., Snopok, P., Soler, F. J. P., Summers, D. J., Tarrant, J., Taylor, I., Tortora, L., Torun, Y., Tsenov, R., Tunnell, C. D., Walaron, K., Watson, S., Wilson, A., Zisman, M. S.

“…A novel single-particle technique to measure emittance has been developed and used to characterise seventeen different muon beams for the Muon Ionisation…”
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High-Resolution Measurements of e^{+}+H_{2}O Total Cross Section by Loreti, A, Kadokura, R, Fayer, S E, Kövér, Á, Laricchia, G

“…Using a purely electrostatic positron beam, the total cross section of positrons scattering from H_{2}O has been measured for the first time with a high…”
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Interactions of positrons & positronium with matter by Fayer, S E

“…The aim of this work is to help and advance the understanding of the interaction of positrons and positronium (Ps) with matter. Knowledge of these interactions…”
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Gaseous $^3$He Nuclear Magnetic Resonance Probe for Cryogenic Environments by Fan, X, Fayer, S. E, Gabrielse, G

“…Review of Scientific Instruments 90, 083107 (2019) Normal nuclear magnetic resonance (NMR) probes cannot be used to make high frequency resolution measurements…”
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Towards an Improved Test of the Standard Model's Most Precise Prediction by Gabrielse, G, Fayer, S. E, Myers, T. G, Fan, X

“…Atoms 7, 45 (2019) The electron and positron magnetic moments are the most precise prediction of the standard model of particle physics. The most accurate…”
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The Vision of Mr. Brand by Fayer, Steve

“…A short story is presented…”
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Dark Matter Search Results from 4.2 Tonne-Years of Exposure of the LUX-ZEPLIN (LZ) Experiment by Aalbers, J, Amarasinghe, C. S, Angelides, N, Armstrong, J. E, Baker, A, Balashov, S, Bang, J, Beattie, K, Biesiadzinski, T. P, Blockinger, G. M, Brew, C. A. J, Brás, P, Buuck, M, Carmona-Benitez, M. C, Chawla, A, Chen, H, Cherwinka, J. J, Coronel, R, Cox, G, Curran, D, Dave, S, Delgaudio, J, Dey, S, Ding, C, Dobson, J. E. Y, Druszkiewicz, E, Eriksen, S. R, Fan, A, Fearon, N. M, Fieldhouse, N, Fiorucci, S, Flaecher, H, Geffre, A, Genovesi, J, Ghag, C, Gokhale, S, van der Grinten, M. G. D, Hall, T. J, Han, S, Hartigan-O'Connor, E, Heuermann, G, Homenides, G. J, Hunt, D, Jacquet, E, Kaboth, A. C, Khazov, A, Khurana, I, Kingston, J, Korolkova, E. V, Kravitz, S, Lesko, K. T, Lin, J, Lindote, A, Lippincott, W. H, Lorenzon, W, Lu, C, Majewski, P. A, Manalaysay, A, Mannino, R. L, Maupin, C, McCarthy, M. E, McDowell, G, McMonigle, R, Mizrachi, E, Murdy, M, Neves, F, Olcina, I, Oyulmaz, K. Y, Palladino, K. J, Pannifer, N. J, Patton, S. J, Perry, E, Qie, Y, Rhyne, C. A, Richards, A, Riffard, Q, Ritchey, E, Rosero, R, Rushton, T, Santone, D, Sazzad, A. B. M. R, Shafer, B, Siniscalco, J, Smith, R, Sorensen, P, Soria, J, Timalsina, M, Trask, M, Vacheret, A, Velan, V, Wang, Y, Watson, J. R, Weeldreyer, L, Whitis, T. J, Wild, K, Wisniewski, W. J, Wolf, L, Woodford, S, Woodward, D, Zha, W

“…We report results of a search for nuclear recoils induced by weakly interacting massive particle (WIMP) dark matter using the LUX-ZEPLIN (LZ) two-phase xenon…”
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Cosmogenic production of $^{37}$Ar in the context of the LUX-ZEPLIN experiment by Aalbers, J, Alsum, S. K, Amarasinghe, C. S, Ames, A, Angelides, N, Araújo, H. M, Armstrong, J. E, Balashov, S, Bang, J, Bernard, E. P, Bhatti, A, Biekert, A, Birch, H. J, Bodnia, E, Boxer, B, Brew, C. A. J, Busenitz, J. K, Cabrita, R, Carmona-Benitez, M. C, Cascella, M, Chawla, A, Chen, H, Chott, N. I, Cole, A, Converse, M. V, Cutter, J. E, de Viveiros, L, Druszkiewicz, E, Fayer, S, Fearon, N. M, Fraser, E. D, Gaitskell, R. J, Genovesi, J, Ghag, C, Gilchriese, M. G. D, van der Grinten, M. G. D, Gwilliam, C. B, Haselschwardt, S. J, Horn, M, Hunt, D, Ignarra, C. M, James, R. S, Ji, W, Johnson, J, Kamaha, A. C, Khaitan, D, Kodroff, D, Korley, L, Kravitz, S, Kreczko, L, Kudryavtsev, V. A, Leason, E. A, Levy, C, Linehan, R, Lippincott, W. H, Liu, X, Asamar, E. Lopez, Manenti, L, Marangou, N, McKinsey, D. N, McLaughlin, J, Mizrachi, E, Monzani, M. E, Morad, J. A, Mendoza, J. D. Morales, Naim, D, Naylor, A, Nikoleyczik, J. A, Nilima, A, Oliver-Mallory, K, Pal, S, Palmer, J, Patton, S. J, Pereira, G, Pershing, J, Porzio, D, Richards, A, Schnee, R. W, Shutt, T. A, Silk, J. J, Silva, C, Sinev, G, Smith, R, Solmaz, M, Soria, J, Stevens, A, Stifter, K, Swanson, N, Szydagis, M, Taylor, R, Temples, D. J, Timalsina, M, To, W. H, Tovey, D. R, Trask, M, Utku, U, Wang, B, Whitis, T. J, Woodward, D, Xia, Q

“…We estimate the amount of $^{37}$Ar produced in natural xenon via cosmic ray-induced spallation, an inevitable consequence of the transportation and storage of…”
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Projected sensitivity of the LUX-ZEPLIN (LZ) experiment to the two-neutrino and neutrinoless double beta decays of $^{134}$Xe by Collaboration, Alsum, S. K, Amarasinghe, C. S, Ames, A, Araujo, H. M, Armstrong, J. E, Arthurs, M, Bai, X, Balashov, S, Bang, J, Beltrame, P, Bernard, E. P, Bhatti, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Blockinger, G. M, Bodnia, E, Boxer, B, Bras, P, Busenitz, J. K, Carmona-Benitez, M. C, Cascella, M, Cole, A, Converse, M. V, Cottle, A, Dahl, C. E, Eriksen, S. R, Fan, A, Fayer, S, Fiorucci, S, Fraser, E. D, Fruth, T, Gokhale, S, van der Grinten, M. G. D, Huang, D. Q, Ignarra, C. M, James, R. S, Ji, W, Kaboth, A. C, Kamaha, A. C, Kazkaz, K, Khurana, I, Kodroff, D, Kudryavtsev, V. A, Levy, C, Liao, J, Lin, J, Lippincott, W. H, Asamar, E. Lopez, Paredes, B. Lopez, Manenti, L, Mannino, R. L, Marangou, N, McLaughlin, J, Miller, E. H, Mizrachi, E, Mendoza, J. D. Morales, Naim, D, Nedlik, C, Nelson, H. N, Nikoleyczik, J. A, Nilima, A, Oliver-Mallory, K. C, Pal, S, Palladino, K. J, Palmer, J, Patton, S, Parveen, N, Penning, B, Pereira, G, Piepke, A, Qie, Y, Riffard, Q, Rossiter, P, Sazzad, A. B. M. R, Schnee, R. W, Scovell, P. R, Shaw, S, Shutt, T. A, Silk, J. J, Silva, C, Smith, R, Sorensen, P, Soria, J, Stifter, K, Swanson, N, Terman, P. A, Timalsina, M, To, W. H, Tovey, D. R, Tripathi, M, Tronstad, D. R, Utku, U, Vaitkus, A, Wang, B, Wang, J. J, Watson, J. R, White, R. G, Wright, C. J

“…The projected sensitivity of the LUX-ZEPLIN (LZ) experiment to two-neutrino and neutrinoless double beta decay of $^{134}$Xe is presented. LZ is a 10-tonne…”
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Projected sensitivities of the LUX-ZEPLIN (LZ) experiment to new physics via low-energy electron recoils by Amarasinghe, C. S, Anderson, T. J, Angelides, N, Armstrong, J. E, Balajthy, J, Bargemann, J. W, Baxter, A, Beltrame, P, Bernstein, A, Biekert, A, Blockinger, G. M, Boxer, B, Brew, C. A. J, Brás, P, Burdin, S, Buuck, M, Cabrita, R, Carmona-Benitez, M. C, Cascella, M, Chan, C, Chott, N. I, Cottle, A, Cox, G, Creaner, O, de Viveiros, L, Dobson, J. E. Y, Eriksen, S. R, Fearon, N. M, Flaecher, H, Gibson, E, Gwilliam, C. B, Hall, C. R, Hardy, C. A, Horn, M, Ignarra, C. M, James, R. S, Ji, W, Kazkaz, K, Khaitan, D, Khurana, I, Kodroff, D, Kravitz, S, Kreczko, L, Leason, E. A, Leonard, D. S, Lesko, K. T, Levy, C, Li, J, Liao, J, Liu, X, Lorenzon, W, Manalaysay, A, Marangou, N, McCarthy, M. E, McLaughlin, J, Miller, E. H, Monzani, M. E, Morad, J. A, Mendoza, J. D. Morales, Naim, D, Nedlik, C, Nelson, H. N, Nguyen, A, Oliver-Mallory, K. C, Pal, S, Palladino, K. J, Palmer, J, Patton, S, Parveen, N, Penning, B, Pereira, G, Piepke, A, Qie, Y, Riffard, Q, Rossiter, P, Sazzad, A. B. M. R, Schnee, R. W, Scovell, P. R, Shaw, S, Shutt, T. A, Silk, J. J, Silva, C, Smith, R, Sorensen, P, Soria, J, Stifter, K, Swanson, N, Terman, P. A, Timalsina, M, To, W. H, Tovey, D. R, Tripathi, M, Tronstad, D. R, Utku, U, Vaitkus, A, Wang, B, Wang, J. J, Watson, J. R, White, R. G, Wright, C. J

“…LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear…”
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Enhancing the sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment to low energy signals by Akerib, D. S, Ames, A, Anderson, T. J, Araújo, H. M, Armstrong, J. E, Arthurs, M, Bai, X, Balashov, S, Bang, J, Bauer, D, Baxter, A, Beltrame, P, Bernard, E. P, Bernstein, A, Biekert, A, Biesiadzinski, T. P, Birch, H. J, Blockinger, G. M, Boxer, B, Brew, C. A. J, Buuck, M, Cabrita, R, Cascella, M, Chan, C, Chott, N. I, Cole, A, Cox, G, Cutter, J. E, Dobson, J. E. Y, Druszkiewicz, E, Flaecher, H, Fruth, T, Genovesi, J, Ghag, C, Gokhale, S, Haselschwardt, S. J, Huang, D. Q, Ignarra, C. M, James, R. S, Ji, W, Kaboth, A. C, Kazkaz, K, Khaitan, D, Khazov, A, Kodroff, D, Korolkova, E. V, Kraus, H, Kudryavtsev, V. A, Levy, C, Li, J, Lin, J, Paredes, B. López, Lorenzon, W, Majewski, P. A, Manalaysay, A, Mannino, R. L, McKinsey, D. N, Mizrachi, E, Morad, J. A, Mendoza, J. D. Morales, Morrison, E, Mount, B. J, Naim, D, Nedlik, C, Nikoleyczik, J. A, Oliver-Mallory, K. C, Pal, S, Palmer, J, Pease, E. K, Penning, B, Pereira, G, Reichenbacher, J, Richards, A, Riffard, Q, Rischbieter, G. R. C, Sazzad, A. B. M. R, Scovell, P. R, Shutt, T. A, Silk, J. J, Silva, C, Solovov, V. N, Sorensen, P, Stancu, I, Stifter, K, Sumner, T. J, Swanson, N, Szydagis, M, Taylor, W. C, Taylor, R, Terman, P. A, Tiedt, D. R, Timalsina, M, To, W. H, Tripathi, M, Wang, B, White, R. G, Williams, M, Woodward, D, Xiang, X, Xu, J

“…Two-phase xenon detectors, such as that at the core of the forthcoming LZ dark matter experiment, use photomultiplier tubes to sense the primary (S1) and…”
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Simulations of Events for the LUX-ZEPLIN (LZ) Dark Matter Experiment by Alsum, S. K, Anderson, T. J, Angelides, N, Armstrong, J. E, Balajthy, J, Bauer, D, Baxter, A, Bernstein, A, Boast, K. E, Brás, P, Bugaev, V. V, Burdin, S, Carels, C, Carlsmith, D. L, Cascella, M, Cutter, J. E, Dahl, C. E, Fayer, S, Fiorucci, S, Fraser, E. D, Fruth, T, Gaitskell, R. J, Genovesi, J, Ghag, C, Gilchriese, M. G. D, van der Grinten, M. G. D, Harrison, A, Haselschwardt, S. J, Hertel, S. A, Horn, M, Jahangir, O, Kaboth, A. C, Kamdin, K, Khaitan, D, Khazov, A, Kocher, C. D, Korley, L, Korolkova, E. V, Kras, J, Kraus, H, Kravitz, S, Kreczko, L, Krikler, B, Leason, E. A, Lee, J, Leonard, D. S, Li, J, Liao, J, Liao, F. -T, Lin, J, Loniewski, C, Manenti, L, Marangou, N, McKinsey, D. N, McLaughlin, J, Mizrachi, E, Monte, A, Monzani, M. E, Morad, J. A, Morrison, E, Mount, B. J, Naim, D, Naylor, A, Nikoleyczik, J. A, Nilima, A, Olcina, I, Oliver-Mallory, K. C, Pal, S, Pereira, G, Piepke, A, Pushkin, K, Rhyne, C. A, Riffard, Q, Rosero, R, Rossiter, P, Santone, D, Schnee, R. W, Schubnell, M, Scovell, P. R, Seymour, D, Shutt, T. A, Solmaz, M, Solovov, V. N, Sorensen, P, Stancu, I, Stevens, A, Szydagis, M, Taylor, W. C, Taylor, R, Temples, D. J, Tomás, A, Tripathi, M, Turner, W, Tvrznikova, L, Utku, U, Wang, J. J, Webb, R. C, Whitis, T. J, Wolfs, F. L. H, Woodward, D

“…The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1--2)$\times10^{-12}$\,pb at a WIMP…”
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