A restricted dimer model on a two-dimensional random causal triangulation

Journal of Physics A: Mathematical and Theoretical IOP Publishing 47:36 (2014) 365001-365001

Authors:

J Ambjørn, B Durhuus, John Wheater

Abstract:

We introduce a restricted hard dimer model on a random causal triangulation that is exactly solvable and generalizes a model recently proposed by Atkin and Zohren (2012 Phys. Lett. B 712 445–50). We show that the latter model exhibits unusual behaviour at its multicritical point; in particular, its Hausdorff dimension equals 3 and not $3/2$ as would be expected from general scaling arguments. When viewed as a special case of the generalized model introduced here we show that this behaviour is not generic and therefore is not likely to represent the true behaviour of the full dimer model on a random causal triangulation.

Leptophilic dark matter and the anomalous magnetic moment of the muon

Journal of High Energy Physics Springer Nature 2014:8 (2014) 147

Authors:

Prateek Agrawal, Zackaria Chacko, Christopher B Verhaaren

3.55 keV photon line and its morphology from a 3.55 keV axionlike particle line

Physical Review D American Physical Society (APS) 90:2 (2014) 023540

Authors:

Michele Cicoli, Joseph P Conlon, MC David Marsh, Markus Rummel

A SEARCH FOR POINT SOURCES OF EeV PHOTONS

The Astrophysical Journal American Astronomical Society 789:2 (2014) 160

Authors:

A Aab, P Abreu, M Aglietta, M Ahlers, EJ Ahn, I Al Samarai, IFM Albuquerque, I Allekotte, J Allen, P Allison, A Almela, J Alvarez Castillo, J Alvarez-Muñiz, R Alves Batista, M Ambrosio, A Aminaei, L Anchordoqui, S Andringa, C Aramo, F Arqueros, H Asorey, P Assis, J Aublin, M Ave, M Avenier, G Avila, AM Badescu, KB Barber, J Bäuml, C Baus, JJ Beatty, KH Becker, JA Bellido, C Berat, X Bertou, PL Biermann, P Billoir, F Blanco, M Blanco, C Bleve, H Blümer, M Boháčová, D Boncioli, C Bonifazi, R Bonino, N Borodai, J Brack, I Brancus, P Brogueira, WC Brown, P Buchholz, A Bueno, M Buscemi, KS Caballero-Mora, B Caccianiga, L Caccianiga, M Candusso, L Caramete, R Caruso, A Castellina, G Cataldi, L Cazon, R Cester, AG Chavez, SH Cheng, A Chiavassa, JA Chinellato, J Chudoba, M Cilmo, RW Clay, G Cocciolo, R Colalillo, L Collica, MR Coluccia, R Conceição, F Contreras, MJ Cooper, S Coutu, CE Covault, A Criss, J Cronin, A Curutiu, R Dallier, B Daniel, S Dasso, K Daumiller, BR Dawson, RM de Almeida, M De Domenico, SJ de Jong, JRT de Mello Neto, I De Mitri, J de Oliveira, V de Souza, L del Peral, O Deligny, H Dembinski, N Dhital, C Di Giulio, A Di Matteo, JC Diaz, ML Díaz Castro, PN Diep, F Diogo, C Dobrigkeit, W Docters, JC D'Olivo, PN Dong, A Dorofeev, Q Dorosti Hasankiadeh, MT Dova, J Ebr, R Engel, M Erdmann, M Erfani, CO Escobar, J Espadanal, A Etchegoyen, P Facal San Luis, H Falcke, K Fang, G Farrar, AC Fauth, N Fazzini, AP Ferguson, M Fernandes, B Fick, JM Figueira, A Filevich, A Filipčič, BD Fox, O Fratu, U Fröhlich, B Fuchs, T Fuji, R Gaior, B García, ST Garcia Roca, D Garcia-Gamez, D Garcia-Pinto, G Garilli, A Gascon Bravo, F Gate, H Gemmeke, PL Ghia, U Giaccari, M Giammarchi, M Giller, C Glaser, H Glass, F Gomez Albarracin, M Gómez Berisso, PF Gómez Vitale, P Gonçalves, JG Gonzalez, B Gookin, A Gorgi, P Gorham, P Gouffon, S Grebe, N Griffith, AF Grillo, TD Grubb, Y Guardincerri, F Guarino, GP Guedes, P Hansen, D Harari, TA Harrison, JL Harton, A Haungs, T Hebbeker, D Heck, P Heimann, AE Herve, GC Hill, C Hojvat, N Hollon, E Holt, P Homola, JR Hörandel, P Horvath, M Hrabovský, D Huber, T Huege, A Insolia, PG Isar, K Islo, I Jandt, S Jansen, C Jarne, M Josebachuili, A Kääpä, O Kambeitz, KH Kampert, P Kasper, I Katkov, B Kégl, B Keilhauer, A Keivani, E Kemp, RM Kieckhafer, HO Klages, M Kleifges, J Kleinfeller, R Krause, N Krohm, O Krömer, D Kruppke-Hansen, D Kuempel, N Kunka, G La Rosa, D LaHurd, L Latronico, R Lauer, M Lauscher, P Lautridou, S Le Coz, MSAB Leão, D Lebrun, P Lebrun, MA Leigui de Oliveira, A Letessier-Selvon, I Lhenry-Yvon, K Link, R López, A Lopez Agüera, K Louedec, J Lozano Bahilo, L Lu, A Lucero, M Ludwig, H Lyberis, MC Maccarone, M Malacari, S Maldera, J Maller, D Mandat, P Mantsch, AG Mariazzi, V Marin, IC Mariş, G Marsella, D Martello, L Martin, H Martinez, O Martínez Bravo, D Martraire, JJ Masías Meza, HJ Mathes, S Mathys, AJ Matthews, J Matthews, G Matthiae, D Maurel, D Maurizio, E Mayotte, PO Mazur, C Medina, G Medina-Tanco, M Melissas, D Melo, E Menichetti, A Menshikov, S Messina, R Meyhandan, S Mićanović, MI Micheletti, L Middendorf, IA Minaya, L Miramonti, B Mitrica, L Molina-Bueno, S Mollerach, M Monasor, D Monnier Ragaigne, F Montanet, C Morello, JC Moreno, M Mostafá, CA Moura, MA Muller, G Müller, M Münchmeyer, R Mussa, G Navarra, S Navas, P Necesal, L Nellen, A Nelles, J Neuser, M Niechciol, L Niemietz, T Niggemann, D Nitz, D Nosek, V Novotny, L Nožka, L Ochilo, A Olinto, M Oliveira, M Ortiz, N Pacheco, D Pakk Selmi-Dei, M Palatka, J Pallotta, N Palmieri, P Papenbreer, G Parente, A Parra, S Pastor, T Paul, M Pech, J Pe¸kala, R Pelayo, IM Pepe, L Perrone, R Pesce, E Petermann, C Peters, S Petrera, A Petrolini, Y Petrov, R Piegaia, T Pierog, P Pieroni, M Pimenta, V Pirronello, M Platino, M Plum, A Porcelli, C Porowski, P Privitera, M Prouza, V Purrello, EJ Quel, S Querchfeld, S Quinn, J Rautenberg, O Ravel, D Ravignani, B Revenu, J Ridky, S Riggi, M Risse, P Ristori, V Rizi, J Roberts, W Rodrigues de Carvalho, I Rodriguez Cabo, G Rodriguez Fernandez, J Rodriguez Rojo, MD Rodríguez-Frías, G Ros, J Rosado, T Rossler, M Roth, E Roulet, AC Rovero, C Rühle, SJ Saffi, A Saftoiu, F Salamida, H Salazar, F Salesa Greus, G Salina, F Sánchez, P Sanchez-Lucas, CE Santo, E Santos, EM Santos, F Sarazin, B Sarkar, R Sarmento, R Sato, N Scharf, V Scherini, H Schieler, P Schiffer, A Schmidt, O Scholten, H Schoorlemmer, P Schovánek, A Schulz, J Schulz, SJ Sciutto, A Segreto, M Settimo, A Shadkam, RC Shellard, I Sidelnik, G Sigl, O Sima, A Śmiałkowski, R Šmída, GR Snow, P Sommers, J Sorokin, R Squartini, YN Srivastava, S Stanič, J Stapleton, J Stasielak, M Stephan, A Stutz, F Suarez, T Suomijärvi, AD Supanitsky, MS Sutherland, J Swain, Z Szadkowski, M Szuba, OA Taborda, A Tapia, M Tartare, NT Thao, VM Theodoro, J Tiffenberg, C Timmermans, CJ Todero Peixoto, G Toma, L Tomankova, B Tomé, A Tonachini, G Torralba Elipe, D Torres Machado, P Travnicek, E Trovato, M Tueros, R Ulrich, M Unger, M Urban, JF Valdés Galicia, I Valiño, L Valore, G van Aar, AM van den Berg, S van Velzen, A van Vliet, E Varela, B Vargas Cárdenas, G Varner, JR Vázquez, RA Vázquez, D Veberič, V Verzi, J Vicha, M Videla, L Villaseñor, B Vlcek, S Vorobiov, H Wahlberg, O Wainberg, D Walz, AA Watson, M Weber, K Weidenhaupt, A Weindl, F Werner, BJ Whelan, A Widom, L Wiencke, B Wilczyńska, H Wilczyński, M Will, C Williams, T Winchen, D Wittkowski, B Wundheiler, S Wykes, T Yamamoto, T Yapici, P Younk, G Yuan, A Yushkov, B Zamorano, E Zas, D Zavrtanik, M Zavrtanik, I Zaw, A Zepeda, J Zhou, Y Zhu, M Zimbres Silva, M Ziolkowski

Search for non-relativistic Magnetic Monopoles with IceCube

European Physical Journal C Springer Verlag C74:7 (2014) 2938-2938

Abstract:

The IceCube Neutrino Observatory is a large Cherenkov detector instrumenting $1\,\mathrm{km}^3$ of Antarctic ice. The detector can be used to search for signatures of particle physics beyond the Standard Model. Here, we describe the search for non-relativistic, magnetic monopoles as remnants of the GUT (Grand Unified Theory) era shortly after the Big Bang. These monopoles may catalyze the decay of nucleons via the Rubakov-Callan effect with a cross section suggested to be in the range of $10^{-27}\,\mathrm{cm^2}$ to $10^{-21}\,\mathrm{cm^2}$. In IceCube, the Cherenkov light from nucleon decays along the monopole trajectory would produce a characteristic hit pattern. This paper presents the results of an analysis of first data taken from May 2011 until May 2012 with a dedicated slow-particle trigger for DeepCore, a subdetector of IceCube. A second analysis provides better sensitivity for the brightest non-relativistic monopoles using data taken from May 2009 until May 2010. In both analyses no monopole signal was observed. For catalysis cross sections of $10^{-22}\,(10^{-24})\,\mathrm{cm^2}$ the flux of non-relativistic GUT monopoles is constrained up to a level of $\Phi_{90} \le 10^{-18}\,(10^{-17})\,\mathrm{cm^{-2}s^{-1}sr^{-1}}$ at a 90% confidence level, which is three orders of magnitude below the Parker bound. The limits assume a dominant decay of the proton into a positron and a neutral pion. These results improve the current best experimental limits by one to two orders of magnitude, for a wide range of assumed speeds and catalysis cross sections.