Low-Threshold Response of a Scintillating Xenon Bubble Chamber to Nuclear and Electronic Recoils

Autor: Alfonso-Pita, E., Behnke, E., Bressler, M., Broerman, B., Clark, K., Coppejans, R., Corbett, J., Crisler, M., Dahl, C. E., Dering, K., Croix, A. de St., Durnford, D., Giampa, P., Hall, J., Harris, O., Hawley-Herrera, H., Lamb, N., Laurin, M., Levine, I., Lippincott, W. H., Neilson, R., Piro, M. -C., Pyda, D., Sheng, Z., Sweeney, G., Vázquez-Jáuregui, E., Westerdale, S., Whitis, T. J., Wright, A., Zhang, J., Zhang, R., Zuñiga-Reyes, A.

A device filled with pure xenon first demonstrated the ability to operate simultaneously as a bubble chamber and scintillation detector in 2017. Initial results from data taken at thermodynamic thresholds down to ~4 keV showed sensitivity to ~20 keV

Externí odkaz: http://arxiv.org/abs/2410.07241

Search for inelastic dark matter-nucleus scattering with the PICO-60 CF$_{3}$I and C$_{3}$F$_{8}$ bubble chambers

Autor: Adams, E., Ali, B., Arnquist, I. J., Baxter, D., Behnke, E., Bressler, M., Broerman, B., Chen, C. J., Clark, K., Collar, J. I., Cooper, P. S., Cripe, C., Crisler, M., Dahl, C. E., Das, M., Fallows, S., Farine, J., Filgas, R., Viltres, A. García, Giroux, G., Harris, O., Hillier, T., Hoppe, E. W., Jackson, C. M., Jin, M., Krauss, C. B., Kumar, V., Laurin, M., Lawson, I., Leblanc, A., Leng, H., Levine, I., Licciardi, C., Lippincott, W. H., Mitra, P., Monette, V., Moore, C., Neilson, R., Noble, A. J., Nozard, H., Pal, S., Piro, M. -C., Plante, A., Priya, S., Rethmeier, C., Robinson, A. E., Savoie, J., Sonnenschein, A., Starinski, N., Štekl, I., Tiwari, D., Vázquez-Jáuregui, E., Wichoski, U., Zacek, V., Zhang, J.

PICO bubble chambers have exceptional sensitivity to inelastic dark matter-nucleus interactions due to a combination of their extended nuclear recoil energy detection window from a few keV to $O$(100 keV) or more and the use of iodine as a heavy targ

Externí odkaz: http://arxiv.org/abs/2301.08993

Determining the bubble nucleation efficiency of low-energy nuclear recoils in superheated C$_3$F$_8$ dark matter detectors

Autor: Ali, B., Arnquist, I. J., Baxter, D., Behnke, E., Bressler, M., Broerman, B., Clark, K., Collar, J. I., Cooper, P. S., Cripe, C., Crisler, M., Dahl, C. E., Das, M., Durnford, D., Fallows, S., Farine, J., Filgas, R., García-Viltres, A., Girard, F., Giroux, G., Harris, O., Hoppe, E. W., Jackson, C. M., Jin, M., Krauss, C. B., Kumar, V., Lafreniere, M., Laurin, M., Lawson, I., Leblanc, A., Leng, H., Levine, I., Licciardi, C., Linden, S., Mitra, P., Monette, V., Moore, C., Neilson, R., Noble, A. J., Nozard, H., Pal, S., Piro, M. -C., Plante, A., Priya, S., Rethmeier, C., Robinson, A. E., Savoie, J., Scallon, O., Sonnenschein, A., Starinski, N., Štekl, I., Tiwari, D., Tardif, F., Vázquez-Jáuregui, E., Wichoski, U., Zacek, V., Zhang, J.

The bubble nucleation efficiency of low-energy nuclear recoils in superheated liquids plays a crucial role in interpreting results from direct searches for weakly interacting massive particle (WIMP) dark matter. The PICO Collaboration presents the re

Externí odkaz: http://arxiv.org/abs/2205.05771

PICASSO, COUPP and PICO - search for dark matter with bubble chambers

Autor: Amole C., Ardid M., Asner D. M., Baxter D., Behnke E., Bhattacharjee P., Borsodi H., Bou-Cabo M., Brice S. J., Broemmelsiek D., Clark K., Collar J. I., Cooper P. S., Crisler M., Dahl C. E., Das M., Debris F., Dhungana N., Farine J., Felis I., Filgas R., Fines-Neuschild M., Girard F., Giroux G., Hai M., Hall J., Harris O., Jackson C. M., Jin M., Krauss C., Lafrenière M., Laurin M., Lawson I., Levine I., Lippincott W. H., Mann E., Martin J. P., Maurya D., Mitra P., Neilson R., Noble A. J., Plante A., Podviyanuk R., Priya S., Robinson A. E., Ruschman M., Scallon O., Seth S., Sonnenschein A., Starinski N., Štekl I., Vázquez-Jáuregui E., Wells J., Wichoski U., Zacek V., Zhang J.

Publikováno v: EPJ Web of Conferences, Vol 95, p 04020 (2015)

The PICASSO and COUPP collaborations use superheated liquid detectors to search for cold dark matter through the direct detection of weakly interacting massive particles (WIMPs). These experiments, located in the underground laboratory of SNOLAB, Can

Externí odkaz: https://doaj.org/article/38c974e257b540a784f5d5e8fecdf1d8

Velocity independent constraints on spin-dependent DM-nucleon interactions from IceCube and PICO

Autor: IceCube Collaboration, Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alispach, C., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argüelles, C., Auffenberg, J., Axani, S., Backes, P., Bagherpour, H., Bai, X., V., A. Balagopal, Barbano, A., Barwick, S. W., Bastian, B., Baum, V., Baur, S., Bay, R., Beatty, J. J., Becker, K. -H., Tjus, J. Becker, BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Börner, M., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Bron, S., Brostean-Kaiser, J., Burgman, A., Buscher, J., Busse, R. S., Carver, T., Chen, C., Cheung, E., Chirkin, D., Choi, S., Classen, L., Coleman, A., Collin, G. H., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dave, P., De Clercq, C., DeLaunay, J. J., Dembinski, H., Deoskar, K., De Ridder, S., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., Diaz, A., Díaz-Vélez, J. C., Dujmovic, H., Dunkman, M., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eller, P., Engel, R., Evenson, P. A., Fahey, S., Fazely, A. R., Felde, J., Filimonov, K., Finley, C., Franckowiak, A., Friedman, E., Fritz, A., Gaisser, T. K., Gallagher, J., Ganster, E., Garrappa, S., Gerhardt, L., Ghorbani, K., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Griffith, Z., Griswold, S., Günder, M., Gündüz, M., Haack, C., Hallgren, A., Halve, L., Halzen, F., Hanson, K., Haungs, A., Hebecker, D., Heereman, D., Heix, P., Helbing, K., Hellauer, R., Henningsen, F., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoinka, T., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Huber, T., Hultqvist, K., Hünnefeld, M., Hussain, R., In, S., Iovine, N., Ishihara, A., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Jonske, F., Joppe, R., Kang, D., Kang, W., Kappes, A., Kappesser, D., Karg, T., Karl, M., Karle, A., Katz, U., Kauer, M., Kelley, J. L., Kheirandish, A., Kim, J., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Koirala, R., Kolanoski, H., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krings, K., Krückl, G., Kulacz, N., Kurahashi, N., Kyriacou, A., Labare, M., Lanfranchi, J. L., Larson, M. J., Lauber, F., Lazar, J. P., Leonard, K., Leszczyńska, A., Leuermann, M., Liu, Q. R., Lohfink, E., Mariscal, C. J. Lozano, Lu, L., Lucarelli, F., Lünemann, J., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Maggi, G., Mahn, K. B. M., Makino, Y., Mallik, P., Mallot, K., Mancina, S., Mariş, I. C., Maruyama, R., Mase, K., Maunu, R., McNally, F., Meagher, K., Medici, M., Medina, A., Meier, M., Meighen-Berger, S., Menne, T., Merino, G., Meures, T., Micallef, J., Mockler, D., Momenté, G., Montaruli, T., Moore, R. W., Morse, R., Moulai, M., Muth, P., Nagai, R., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Pollmann, A. Obertacke, Oehler, M., Olivas, A., O'Murchadha, A., O'Sullivan, E., Palczewski, T., Pandya, H., Pankova, D. V., Park, N., Peiffer, P., Heros, C. Pérez de los, Philippen, S., Pieloth, D., Pinat, E., Pizzuto, A., Plum, M., Porcelli, A., Price, P. B., Przybylski, G. T., Raab, C., Raissi, A., Rameez, M., Rauch, L., Rawlins, K., Rea, I. C., Reimann, R., Relethford, B., Renschler, M., Renzi, G., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Safa, I., Herrera, S. E. Sanchez, Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Schaufel, M., Schieler, H., Schlunder, P., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Sclafani, S., Seckel, D., Seunarine, S., Shefali, S., Silva, M., Snihur, R., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stein, R., Steinmüller, P., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Strotjohann, N. L., Stürwald, T., Stuttard, T., Sullivan, G. W., Taboada, I., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tilav, S., Tomankova, L., Tönnis, C., Toscano, S., Tosi, D., Trettin, A., Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Turley, C. F., Ty, B., Unger, E., Elorrieta, M. A. Unland, Usner, M., Vandenbroucke, J., Van Driessche, W., van Eijk, D., van Eijndhoven, N., Vanheule, S., van Santen, J., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Watson, T. B., Weaver, C., Weindl, A., Weiss, M. J., Weldert, J., Wendt, C., Werthebach, J., Whelan, B. J., Whitehorn, N., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wolf, M., Wood, J., Wood, T. R., Woschnagg, K., Wrede, G., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T., Collaboration, M. Zöcklein. PICO, Amole, C., Ardid, M., Arnquist, I. J., Asner, D. M., Baxter, D., Behnke, E., Bressler, M., Broerman, B., Cao, G., Chen, C. J., Chowdhury, U., Clark, K., Collar, J. I., Cooper, P. S., Crisler, M., Crowder, G., Cruz-Venegas, N. A., Dahl, C. E., Das, M., Fallows, S., Farine, J., Felis, I., Filgas, R., Girard, F., Giroux, G., Hall, J., Hardy, C., Harris, O., Hoppe, E. W., Jin, M., Klopfenstein, L., Krauss, C. B., Laurin, M., Lawson, I., Leblanc, A., Levine, I., Lippincott, W. H., Mamedov, F., Maurya, D., Mitra, P., Moore, C., Nania, T., Neilson, R., Noble, A. J., Oedekerk, P., Ortega, A., Piro, M. -C., Plante, A., Podviyanuk, R., Priya, S., Robinson, A. E., Sahoo, S., Scallon, O., Seth, S., Sonnenschein, A., Starinski, N., Štekl, I., Sullivan, T., Tardif, F., Vázquez-Jáuregui, E., Walkowski, N., Wichoski, U., Yan, Y., Zacek, V., Zhang, J.

Publikováno v: Eur. Phys. J. C 80 (2020) 819

Adopting the Standard Halo Model (SHM) of an isotropic Maxwellian velocity distribution for dark matter (DM) particles in the Galaxy, the most stringent current constraints on their spin-dependent scattering cross-section with nucleons come from the

Externí odkaz: http://arxiv.org/abs/1907.12509