P
P. Mitra
Researcher at University of Alberta
Publications - 24
Citations - 1110
P. Mitra is an academic researcher from University of Alberta. The author has contributed to research in topics: Dark matter & Weakly interacting massive particles. The author has an hindex of 8, co-authored 13 publications receiving 920 citations.
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Journal ArticleDOI
Dark Matter Search Results from the PICO-60C(3)F(8) Bubble Chamber
C. Amole,M. Ardid,I. J. Arnquist,D. M. Asner,D. Baxter,E. Behnke,Pijushpani Bhattacharjee,H. Borsodi,Manuel Bou-Cabo,P. Campion,G. Cao,Chujie Chen,U. Chowdhury,Karl J. Clark,J. I. Collar,P. S. Cooper,M. B. Crisler,G. Crowder,C. E. Dahl,Mala Das,S. Fallows,J. Farine,Ivan Felis,R. Filgas,F. Girard,G. Giroux,J. Hall,O. Harris,Eric W. Hoppe,M. Jin,C. B. Krauss,M. Laurin,I. Lawson,A. Leblanc,Ilan Levine,W. H. Lippincott,F. Mamedov,Deepam Maurya,P. Mitra,T. Nania,R. Neilson,A. J. Noble,S. Olson,Amber M. Ortega,A. Plante,R. Podviyanuk,Shashank Priya,A. E. Robinson,A. Roeder,R. Rucinski,O. Scallon,Satyajit Seth,A. Sonnenschein,N. Starinski,I. Stekl,F. Tardif,E. Vázquez-Jáuregui,J. Wells,U. Wichoski,Yongke Yan,V. Zacek,Jie Zhang +61 more
TL;DR: These results set the most stringent direct-detection constraint to date on the weakly interacting massive particle (WIMP)-proton spin-dependent cross section at 3.4×10^{-41} cm^{2} for a 30-GeV c^{-2} WIMP, more than 1 order of magnitude improvement from previous PICO results.
Journal ArticleDOI
Constraints on Low-Mass WIMP Interactions on $^{19}F$ from PICASSO
S. Archambault,E. Behnke,Pijushpani Bhattacharjee,S. Bhattacharya,X. Dai,Mala Das,A. Davour,F. Debris,N. Dhungana,J. Farine,S. Gagnebin,G. Giroux,E. Grace,C. M. Jackson,A. Kamaha,C. B. Krauss,S. Kumaratunga,M. Lafrenière,M. Laurin,I. Lawson,L. Lessard,I. Levine,C. Levy,R. MacDonald,D. Marlisov,J. P. Martin,P. Mitra,A. J. Noble,M.-C. Piro,R. Podviyanuk,Stanislav Pospisil,Satyajit Saha,O. Scallon,S. Seth,N. Starinski,I. Stekl,U. Wichoski,T. Xie,V. Zacek +38 more
TL;DR: In this article, the PICASSO dark matter search experiment at SNOLAB was used to detect weakly interacting massive particles (WIMPs) with masses below 10 GeV/c 2.
Journal ArticleDOI
Dark Matter Search Results from the Complete Exposure of the PICO-60 C$_3$F$_8$ Bubble Chamber
C. Amole,M. Ardid,I. J. Arnquist,D. M. Asner,D. Baxter,E. Behnke,M. Bressler,B. Broerman,G. Cao,Chujie Chen,U. Chowdhury,Karl J. Clark,J. I. Collar,P. S. Cooper,C. B. Coutu,C. Cowles,M. B. Crisler,G. Crowder,N. A. Cruz-Venegas,C. E. Dahl,Mala Das,S. Fallows,J. Farine,Ivan Felis,R. Filgas,F. Girard,G. Giroux,J. Hall,C. Hardy,O. Harris,T. Hillier,Eric W. Hoppe,C. M. Jackson,M. Jin,L. Klopfenstein,T. Kozynets,C. B. Krauss,M. Laurin,I. Lawson,A. Leblanc,Ilan Levine,C. Licciardi,W. H. Lippincott,B. Loer,F. Mamedov,P. Mitra,C. D. Moore,T. Nania,R. Neilson,A. J. Noble,P. Oedekerk,Amber M. Ortega,M.-C. Piro,A. Plante,R. Podviyanuk,Shashank Priya,A. E. Robinson,S. Sahoo,O. Scallon,Satyajit Seth,A. Sonnenschein,N. Starinski,I. Stekl,T. Sullivan,F. Tardif,E. Vázquez-Jáuregui,N. Walkowski,E. Weima,U. Wichoski,K. Wierman,Yongke Yan,V. Zacek,Jie Zhang +72 more
TL;DR: The PICO Collaboration as discussed by the authors has been supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site.
Journal ArticleDOI
Improved dark matter search results from PICO-2L Run 2
C. Amole,Miguel Ardid,I. J. Arnquist,D. M. Asner,D. Baxter,E. Behnke,Pijushpani Bhattacharjee,H. Borsodi,Manuel Bou-Cabo,S. J. Brice,Daniel Broemmelsiek,K. Clark,J. I. Collar,P. S. Cooper,M. B. Crisler,C. E. Dahl,C. E. Dahl,Mala Das,F. Debris,S. Fallows,J. Farine,Ivan Felis,R. Filgas,M. Fines-Neuschild,F. Girard,F. Girard,G. Giroux,J. Hall,O. Harris,Eric W. Hoppe,C. M. Jackson,M. Jin,C. B. Krauss,M. Lafrenière,M. Laurin,I. Lawson,A. Leblanc,I. Levine,W. H. Lippincott,E. Mann,J. P. Martin,Deepam Maurya,P. Mitra,S. Olson,R. Neilson,A. J. Noble,A. Plante,R. B. Podviianiuk,Shashank Priya,A. E. Robinson,M. Ruschman,O. Scallon,O. Scallon,Andrew Sonnenschein,N. Starinski,I. Stekl,E. Vázquez-Jáuregui,J. Wells,U. Wichoski,V. Zacek,Jie Zhang +60 more
TL;DR: In this article, the PICO Collaboration thanks SNOLAB for their exceptional laboratory space and technical support, and also thanks Fermi National Accelerator Laboratory (Contract No. DE-AC02-07CH11359) and Pacific Northwest National Laboratory for their support.
Journal ArticleDOI
Final results of the PICASSO dark matter search experiment
E. Behnke,M. Besnier,Pijushpani Bhattacharjee,X. Dai,X. Dai,Mala Das,A. Davour,F. Debris,N. Dhungana,J. Farine,M. Fines-Neuschild,S. Gagnebin,G. Giroux,E. Grace,E. Grace,C. M. Jackson,C. M. Jackson,A. Kamaha,C. B. Krauss,M. Lafrenière,M. Laurin,I. T. Lawson,L. Lessard,Ilan Levine,D. Marlisov,J. P. Martin,P. Mitra,A. J. Noble,A. Plante,R. Podviyanuk,Stanislav Pospisil,O. Scallon,S. Seth,S. Seth,N. Starinski,I. Stekl,U. Wichoski,V. Zacek +37 more
TL;DR: The PICASSO dark matter search experiment operated an array of 32 superheated droplet detectors containing 3.0 kg of C 4 F 10 and collected an exposure of 231.4 kgd at SNOLAB between March 2012 and January 2014 as discussed by the authors.