Scale of dark QCD

被引:90
作者
Bai, Yang [1 ]
Schwaller, Pedro [2 ,3 ]
机构
[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
[2] Argonne Natl Lab, HEP Div, Argonne, IL 60439 USA
[3] Univ Illinois, Dept Phys, Chicago, IL 60607 USA
来源
PHYSICAL REVIEW D | 2014年 / 89卷 / 06期
基金
美国国家科学基金会;
关键词
MATTER; BARYOGENESIS; LEPTOGENESIS; ENERGY; BARYON; NUMBER;
D O I
10.1103/PhysRevD.89.063522
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Most of the mass of ordinary matter has its origin from quantum chromodynamics (QCD). A similar strong dynamics, dark QCD, could exist to explain the mass origin of dark matter. Using infrared fixed points of the two gauge couplings, we provide a dynamical mechanism that relates the dark QCD confinement scale to our QCD scale, and hence provides an explanation for comparable dark baryon and proton masses. Together with a mechanism that generates equal amounts of dark baryon and ordinary baryon asymmetries in the early Universe, the similarity of dark matter and ordinary matter energy densities can be naturally explained. For a large class of gauge group representations, the particles charged under both QCD and dark QCD, necessary ingredients for generating the infrared fixed points, are found to have masses at 1-2 TeV, which sets the scale for dark matter direct detection and novel collider signatures involving visible and dark jets.
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页数:7
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共 48 条
[1]   Planck 2013 results. XVI. Cosmological parameters [J].
Ade, P. A. R. ;
Aghanim, N. ;
Armitage-Caplan, C. ;
Arnaud, M. ;
Ashdown, M. ;
Atrio-Barandela, F. ;
Aumont, J. ;
Baccigalupi, C. ;
Banday, A. J. ;
Barreiro, R. B. ;
Bartlett, J. G. ;
Battaner, E. ;
Benabed, K. ;
Benoit, A. ;
Benoit-Levy, A. ;
Bernard, J. -P. ;
Bersanelli, M. ;
Bielewicz, P. ;
Bobin, J. ;
Bock, J. J. ;
Bonaldi, A. ;
Bond, J. R. ;
Borrill, J. ;
Bouchet, F. R. ;
Bridges, M. ;
Bucher, M. ;
Burigana, C. ;
Butler, R. C. ;
Calabrese, E. ;
Cappellini, B. ;
Cardoso, J. -F. ;
Catalano, A. ;
Challinor, A. ;
Chamballu, A. ;
Chary, R. -R. ;
Chen, X. ;
Chiang, H. C. ;
Chiang, L. -Y ;
Christensen, P. R. ;
Church, S. ;
Clements, D. L. ;
Colombi, S. ;
Colombo, L. P. L. ;
Couchot, F. ;
Coulais, A. ;
Crill, B. P. ;
Curto, A. ;
Cuttaia, F. ;
Danese, L. ;
Davies, R. D. .
ASTRONOMY & ASTROPHYSICS, 2014, 571
[2]   Leptogenesis as a common origin for matter and dark matter [J].
An, Haipeng ;
Chen, Shao-Long ;
Mohapatra, Rabindra N. ;
Zhang, Yue .
JOURNAL OF HIGH ENERGY PHYSICS, 2010, (03)
[3]   Search for Light Dark Matter in XENON10 Data [J].
Angle, J. ;
Aprile, E. ;
Arneodo, F. ;
Baudis, L. ;
Bernstein, A. ;
Bolozdynya, A. I. ;
Coelho, L. C. C. ;
Dahl, C. E. ;
DeViveiros, L. ;
Ferella, A. D. ;
Fernandes, L. M. P. ;
Fiorucci, S. ;
Gaitskell, R. J. ;
Giboni, K. L. ;
Gomez, R. ;
Hasty, R. ;
Kastens, L. ;
Kwong, J. ;
Lopes, J. A. M. ;
Madden, N. ;
Manalaysay, A. ;
Manzur, A. ;
McKinsey, D. N. ;
Monzani, M. E. ;
Ni, K. ;
Oberlack, U. ;
Orboeck, J. ;
Plante, G. ;
Santorelli, R. ;
dos Santos, J. M. F. ;
Schulte, S. ;
Shagin, P. ;
Shutt, T. ;
Sorensen, P. ;
Winant, C. ;
Yamashita, M. .
PHYSICAL REVIEW LETTERS, 2011, 107 (05)
[4]  
[Anonymous], ATLASCONF2012109
[5]  
[Anonymous], J HIGH ENERGY PHYS
[6]   Lattice calculation of composite dark matter form factors [J].
Appelquist, T. ;
Brower, R. C. ;
Buchoff, M. I. ;
Cheng, M. ;
Cohen, S. D. ;
Fleming, G. T. ;
Kiskis, J. ;
Lin, M. F. ;
Neil, E. T. ;
Osborn, J. C. ;
Rebbi, C. ;
Schaich, D. ;
Schroeder, C. ;
Syritsyn, S. ;
Voronov, G. ;
Vranas, P. ;
Wasem, J. .
PHYSICAL REVIEW D, 2013, 88 (01)
[7]   Weakly interacting stable hidden sector pions [J].
Bai, Yang ;
Hill, Richard J. .
PHYSICAL REVIEW D, 2010, 82 (11)
[8]   ON THE PHASE-STRUCTURE OF VECTOR-LIKE GAUGE-THEORIES WITH MASSLESS FERMIONS [J].
BANKS, T ;
ZAKS, A .
NUCLEAR PHYSICS B, 1982, 196 (02) :189-204
[9]   BARYOGENESIS, SPHALERONS, AND THE COGENERATION OF DARK MATTER [J].
BARR, SM .
PHYSICAL REVIEW D, 1991, 44 (10) :3062-3066
[10]   ELECTROWEAK FERMION NUMBER VIOLATION AND THE PRODUCTION OF STABLE PARTICLES IN THE EARLY UNIVERSE [J].
BARR, SM ;
CHIVUKULA, RS ;
FARHI, E .
PHYSICS LETTERS B, 1990, 241 (03) :387-391