New upper limit on the decay η→e+e- by Browder, T, Li, F, Li, Y, Rodriguez, J, Bergfeld, T, Eisenstein, B, Ernst, J, Gladding, G, Gollin, G, Hans, R, Johnson, E, Karliner, I, Marsh, M, Palmer, M, Selen, M, Thaler, J, Edwards, K, Bellerive, A, Janicek, R, MacFarlane, D, McLean, K, Patel, P, Sadoff, A, Ammar, R, Baringer, P

“…The application of conventional elementary particle theory to this decay predicts a branching fraction of about 10-9.…”

Light concentrators for the Sudbury Neutrino Observatory by Doucas, G, Gil, S, Jelley, N, McGarry, L, Moorhead, M, Tanner, N, Waltham, C

“…There is an important and growing class of elementary particle detectors which are characterized by a large sensitive volume (thousands of tonnes), very low radioactive backgrounds, and rely on the emission of light for particle detection. …”

Brilliant X-rays using a two-stage plasma insertion device by Holloway, J, Norreys, P, Thomas, A, Bartolini, R, Bingham, R, Nydell, J, Trines, R, Walker, R, Wing, M

“…Particle accelerators have made an enormous impact in all fields of natural sciences, from elementary particle physics, to the imaging of proteins and the development of new pharmaceuticals. …”

Combination of the top-quark mass measurements from the Tevatron collider by Cdf, T, collaborations, D, Aaltonen, T, Abazov, V, Abbott, B, Acharya, B, Adams, M, Adams, T, Alexeev, G, Alkhazov, G, Alton, A, Gonzalez, B, Alverson, G, Amerio, S, Amidei, D, Anastassov, A, Annovi, A, Antos, J, Apollinari, G, Appel, J, Arisawa, T, Artikov, A, Asaadi, J, Ashmanskas, W, Askew, A

“…The top quark is the heaviest known elementary particle, with a mass about 40 times larger than the mass of its isospin partner, the bottom quark. …”

The CRESST Dark Matter Search by Seidel, W, Bravin, M, Bruckmayer, M, Bucci, C, Cooper, S, Distefano, P, Feilitzsch, F, Frank, T, Jochum, J, Keeling, R, Kraus, H, Loidl, M, Marchese, J, Meier, O, Meunier, P, Nagel, U, Pergolesi, D, Pröbst, F, Ramachers, Y, Schnagl, J, Sergeyev, I, Sisti, M, Stodolsky, L, Uchaikin, S, Zerle, L

“…In the search for elementary particle dark matter, CRESST is presently the most advanced deep underground, low-background, cryogenic facility. …”

The CRESST dark matter search by Bravin, M, Bruckmayer, M, Bucci, C, Cooper, S, Giordano, S, von Feilitzsch, F, Hohne, J, Jochum, J, Jorgens, V, Keeling, R, Kraus, H, Loidl, M, Lush, J, Macallister, J, Marchese, J, Meier, O, Meunier, P, Nagel, U, Nussle, T, Probst, F, Ramachers, Y, Sarsa, M, Schnagl, J, Seidel, W, Sergeyev, I

“…In the search for elementary particle dark matter, CRESST is presently the most advanced deep underground, low background, cryogenic facility. …”

Search for maximal flavor violating scalars in same-charge lepton pairs in pp collisions at sqrt[s]=1.96 TeV. by Aaltonen, T, Adelman, J, Akimoto, T, Albrow, MG, Alvarez González, B, Amerio, S, Amidei, D, Anastassov, A, Annovi, A, Antos, J, Aoki, M, Apollinari, G, Apresyan, A, Arisawa, T, Artikov, A, Ashmanskas, W, Attal, A, Aurisano, A, Azfar, F, Azzi-Bacchetta, P, Azzurri, P, Bacchetta, N, Badgett, W, Barbaro-Galtieri, A, Barnes, V

“…Models of maximal flavor violation (MxFV) in elementary particle physics may contain at least one new scalar SU(2) doublet field Phi(FV)=(eta(0),eta(+)) that couples the first and third generation quarks (q_(1), q_(3)) via a Lagrangian term L(FV)=xi(13)Phi(FV)q(1)q(3). …”

Search for maximal flavor violating scalars in same-charge lepton pairs in pp̄ collisions at s=1.96TeV by Aaltonen, T, Adelman, J, Akimoto, T, Albrow, MG, Álvarez González, B, Amerio, S, Amidei, D, Anastassov, A, Annovi, A, Antos, J, Aoki, M, Apollinari, G, Apresyan, A, Arisawa, T, Artikov, A, Ashmanskas, W, Attal, A, Aurisano, A, Azfar, F, Azzi-Bacchetta, P, Azzurri, P, Bacchetta, N, Badgett, W, Barbaro-Galtieri, A, Barnes, V

“…Models of maximal flavor violation (MxFV) in elementary particle physics may contain at least one new scalar SU(2) doublet field ΦFV=(η0,η+) that couples the first and third generation quarks (q1, q3) via a Lagrangian term LFV=ξ13ΦFVq1q3. …”

Constraint on the matter-antimatter symmetry-violating phase in neutrino oscillations by Abe, K, Akutsu, R, Ali, A, Alt, C, Andreopoulos, C, Anthony, L, Antonova, M, Aoki, S, Ariga, A, Asada, Y, Ashida, Y, Atkin, ET, Awataguchi, Y, Ban, S, Barbi, M, Barker, GJ, Barr, G, Barry, C, Batkiewicz-Kwasniak, M, Beloshapkin, A, Bench, F, Berardi, V, Berkman, S, Berns, L, Bhadra, S, Bienstock, S, Blondel, A, Bolognesi, S, Bourguille, B, Boyd, SB, Brailsford, D, Bravar, A, Berguño, DB, Bronner, C, Bubak, A, Avanzini, MB, Calcutt, J, Campbell, T, Cao, S, Cartwright, SL, Catanesi, MG, Cervera, A, Chappell, A, Checchia, C, Cherdack, D, Chikuma, N, Christodoulou, G, Coleman, J, Collazuol, G, Cook, L, Coplowe, D, Cudd, A, Dabrowska, A, Rosa, GD, Dealtry, T, Denner, PF, Dennis, SR, Densham, C, Lodovico, FD, Dokania, N, Dolan, S, Drapier, O, Dumarchez, J, Dunne, P, Eklund, L, Emery-Schrenk, S, Ereditato, A, Fernandez, P, Feusels, T, Finch, AJ, Fiorentini, GA, Fiorillo, G, Francois, C, Friend, M, Fujii, Y, Fujita, R, Fukuda, D, Fukuda, R, Fukuda, Y, Gameil, K, Giganti, C, Golan, T, Gonin, M, Gorin, A, Guigue, M, Hadley, DR, Haigh, JT, Hamacher-Baumann, P, Hartz, M, Hasegawa, T, Hastings, NC, Hayashino, T, Hayato, Y, Hiramoto, A, Hogan, M, Holeczek, J, Van, NTH, Iacob, F, Ichikawa, AK, Ikeda, M, Ishida, T, Ishii, T, Ishitsuka, M, Iwamoto, K, Izmaylov, A, Jamieson, B, Jenkins, SJ, Jesús-Valls, C, Jiang, M, Johnson, S, Jonsson, P, Jung, CK, Kabirnezhad, M, Kaboth, AC, Kajita, T, Kakuno, H, Kameda, J, Karlen, D, Kasetti, SP, Kataoka, Y, Katori, T, Kato, Y, Kearns, E, Khabibullin, M, Khotjantsev, A, Kikawa, T, Kim, H, Kim, J, King, S, Kisiel, J, Knight, A, Knox, A, Kobayashi, T, Koch, L, Koga, T, Konaka, A, Kormos, LL, Koshio, Y, Kowalik, K, Kubo, H, Kudenko, Y, Kukita, N, Kuribayashi, S, Kurjata, R, Kutter, T, Kuze, M, Labarga, L, Lagoda, J, Lamoureux, M, Laveder, M, Lawe, M, Licciardi, M, Lindner, T, Litchfield, RP, Liu, SL, Li, X, Longhin, A, Ludovici, L, Lu, X, Lux, T, Machado, LN, Magaletti, L, Mahn, K, Malek, M, Manly, S, Maret, L, Marino, AD, Martin, JF, Maruyama, T, Matsubara, T, Matsushita, K, Matveev, V, Mavrokoridis, K, Mazzucato, E, McCarthy, M, McCauley, N, McFarland, KS, McGrew, C, Mefodiev, A, Metelko, C, Mezzetto, M, Minamino, A, Mineev, O, Mine, S, Miura, M, Bueno, LM, Moriyama, S, Morrison, J, Mueller, TA, Munteanu, L, Murphy, S, Nagai, Y, Nakadaira, T, Nakahata, M, Nakajima, Y, Nakamura, A, Nakamura, KG, Nakamura, K, Nakayama, S, Nakaya, T, Nakayoshi, K, Nantais, C, Ngoc, TV, Niewczas, K, Nishikawa, K, Nishimura, Y, Nonnenmacher, TS, Nova, F, Novella, P, Nowak, J, Nugent, JC, O'Keeffe, HM, O'Sullivan, L, Odagawa, T, Okumura, K, Okusawa, T, Oser, SM, Owen, RA, Oyama, Y, Palladino, V, Palomino, JL, Paolone, V, Parker, WC, Paudyal, P, Pavin, M, Payne, D, Penn, GC, Pickering, L, Pidcott, C, Pintaudi, G, Guerra, ESP, Pistillo, C, Popov, B, Porwit, K, Posiadala-Zezula, M, Pritchard, A, Quilain, B, Radermacher, T, Radicioni, E, Radics, B, Ratoff, PN, Reinherz-Aronis, E, Riccio, C, Rondio, E, Roth, S, Rubbia, A, Ruggeri, AC, Rychter, A, Sakashita, K, Sánchez, F, Schloesser, CM, Scholberg, K, Schwehr, J, Scott, M, Seiya, Y, Sekiguchi, T, Sekiya, H, Sgalaberna, D, Shah, R, Shaikhiev, A, Shaker, F, Shaykina, A, Shiozawa, M, Shorrock, W, Shvartsman, A, Smirnov, A, Smy, M, Sobczyk, JT, Sobel, H, Soler, FJP, Sonoda, Y, Steinmann, J, Suvorov, S, Suzuki, A, Suzuki, SY, Suzuki, Y, Sztuc, AA, Tada, M, Tajima, M, Takeda, A, Takeuchi, Y, Tanaka, HK, Tanaka, HA, Tanaka, S, Thompson, LF, Toki, W, Touramanis, C, Tsui, KM, Tsukamoto, T, Tzanov, M, Uchida, Y, Uno, W, Vagins, M, Valder, S, Vallari, Z, Vargas, D, Vasseur, G, Vilela, C, Vinning, WGS, Vladisavljevic, T, Volkov, VV, Wachala, T, Walker, J, Walsh, JG, Wang, Y, Wark, D, Wascko, MO, Weber, A, Wendell, R, Wilking, MJ, Wilkinson, C, Wilson, JR, Wilson, RJ, Wood, K, Wret, C, Yamada, Y, Yamamoto, K, Yanagisawa, C, Yang, G, Yano, T, Yasutome, K, Yen, S, Yershov, N, Yokoyama, M, Yoshida, T, Yu, M, Zalewska, A, Zalipska, J, Zaremba, K, Zarnecki, G, Ziembicki, M, Zimmerman, ED, Zito, M, Zsoldos, S, Zykova, A

“…So far, CP violation has not been observed in non-quark elementary particle systems. It has been shown that CP violation in leptons could generate the matter–antimatter disparity through a process called leptogenesis4. …”

The Sudbury Neutrino Observatory by Jelley, N, McDonald, AB, Robertson, R

“…The solar models were vindicated, and the Standard Model of elementary particles and fields had to be revised. Here we present an account of the SNO project, its conclusions to date, and its ongoing analysis. …”

High-precision measurement of the W boson mass with the CDF II detector by Aaltonen, T, Amerio, S, Amidei, D, Anastassov, A, Annovi, A, Antos, J, Apollinari, G, Appel, JA, Arisawa, T, Artikov, A, Asaadi, J, Ashmanskas, W, Auerbach, B, Aurisano, A, Azfar, F, Badgett, W, Bae, T, Barbaro-Galtieri, A, Barnes, VE, Barnett, BA, Barria, P, Bartos, P, Bauce, M, Bedeschi, F, Behari, S, Bellettini, G, Bellinger, J, Benjamin, D, Beretvas, A, Bhatti, A, Bland, KR, Blumenfeld, B, Bocci, A, Bodek, A, Bortoletto, D, Boudreau, J, Boveia, A, Brigliadori, L, Bromberg, C, Brucken, E, Budagov, J, Budd, HS, Burkett, K, Busetto, G, Bussey, P, Butti, P, Buzatu, A, Calamba, A, Camarda, S, Farrington, S, Hays, C, Oakes, L, Renton, P, Et al.

“…The mass of the W boson, a mediator of the weak force between elementary particles, is tightly constrained by the symmetries of the standard model of particle physics. …”

CaWO4 crystals as scintillators for cryogenic dark matter search by Ninković, J, Angloher, G, Bucci, C, Cozzini, C, Frank, T, Hauff, D, Kraus, H, Majorovits, B, Mikhailik, V, Petricca, F, Pröbst, F, Ramachers, Y, Rau, W, Seidel, W, Uchaikin, S

“…The Cryogenic Rare Event Search using Superconducting Thermometers (CRESST II) experiment looks for hypothetical massive elementary particles called Weakly Interacting Massive Particles (WIMPs). …”

Magnetic monopole noise by Dusad, R, Kirschner, F, Hoke, J, Roberts, B, Eyal, A, Flicker, F, Luke, G, Blundell, S, Davis, J

“…Magnetic monopoles1-3 are hypothetical elementary particles with quantized magnetic charge. In principle, a magnetic monopole can be detected by the quantized jump in magnetic flux that it generates upon passage through a superconducting quantum interference device (SQUID)4. …”