Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Alexander M. Wijangco"'
Publikováno v:
Physics Letters B, Vol 781, Iss , Pp 473-479 (2018)
WIMP-nucleon scattering is analyzed at order 1/M in Heavy WIMP Effective Theory. The 1/M power corrections, where M≫mW is the WIMP mass, distinguish between different underlying UV models with the same universal limit and their impact on direct det
Externí odkaz:
https://doaj.org/article/5c950f14d3704d2891d9a4fa6ffe2e84
Publikováno v:
Journal of High Energy Physics, Vol 2017, Iss 6, Pp 1-31 (2017)
Abstract Vector-like fermions charged under both the Standard Model and a new dark gauge group arise in many theories of new physics. If these fermions include an electroweak doublet and singlet with equal dark charges, they can potentially connect t
Externí odkaz:
https://doaj.org/article/7bcdbb9d2cd54de281ec4fe486135f70
Publikováno v:
Physics Letters
Physics Letters B, Vol 781, Iss, Pp 473-479 (2018)
Physics Letters B, Vol 781, Iss, Pp 473-479 (2018)
WIMP-nucleon scattering is analyzed at order $1/M$ in Heavy WIMP Effective Theory. The $1/M$ power corrections, where $M\gg m_W$ is the WIMP mass, distinguish between different underlying UV models with the same universal limit and their impact on di
Publikováno v:
Journal of High Energy Physics, Vol 2017, Iss 6, Pp 1-31 (2017)
Journal of High Energy Physics
Journal of High Energy Physics
Vector-like fermions charged under both the Standard Model and a new dark gauge group arise in many theories of new physics. If these fermions include an electroweak doublet and singlet with equal dark charges, they can potentially connect to the Hig
Publikováno v:
Physics of the Dark Universe. 2(1):17-21
We explore theories of dark matter in which dark matter annihilations produce mono-energetic gamma rays ("lines") in the context of effective field theory, which captures the physics for cases in which the particles mediating the interaction are some
Autor:
Daniel McKinsey, William Shepherd, James Buckley, Alexander M. Wijangco, Ahmed Ismail, R.C. Cotta, JoAnne L. Hewett, Alex Drlica-Wagner, Manoj Kaplinghat, Konstantin Matchev, D. A. Bauer, Jonathan L. Feng, Dan Hooper, Alexander Kusenko, Matthew Cahill-Rowley, Tom Rizzo, Tim M. P. Tait, Matthew Wood, Stefan Funk
Publikováno v:
Bauer, D; Buckley, J; Cahill-Rowley, M; Cotta, R; Drlica-Wagner, A; Feng, JL; et al.(2015). Dark matter in the coming decade: Complementary paths to discovery and beyond. Physics of the Dark Universe, 7-8, 16-23. doi: 10.1016/j.dark.2015.04.001. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/5s49x6cx
Physics of the Dark Universe, vol 7-8, iss 8
Bauer, D; Buckley, J; Cahill-Rowley, M; Cotta, R; Drlica-Wagner, A; Feng, JL; et al.(2017). Dark Matter in the Coming Decade: Complementary Paths to Discovery and Beyond. Phys. Dark Univ., 7(8), 16-23. doi: 10.1016/j.dark.2015.04.001. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/8wm7q87z
Physics of the Dark Universe, vol 7-8, iss 8
Bauer, D; Buckley, J; Cahill-Rowley, M; Cotta, R; Drlica-Wagner, A; Feng, JL; et al.(2017). Dark Matter in the Coming Decade: Complementary Paths to Discovery and Beyond. Phys. Dark Univ., 7(8), 16-23. doi: 10.1016/j.dark.2015.04.001. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/8wm7q87z
In this report we summarize the many dark matter searches currently being pursued through four complementary approaches: direct detection, indirect detection, collider experiments, and astrophysical probes. The essential features of broad classes of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c3ed2f039192cf2e61b1bd9d244a4f68
http://www.escholarship.org/uc/item/5s49x6cx
http://www.escholarship.org/uc/item/5s49x6cx
Autor:
Philip Tanedo, Arvind Rajaraman, Anthony DiFranzo, Alexander M. Wijangco, Tim M. P. Tait, Mohammad Abdullah
We present simplified models for the galactic center gamma-ray excess where Dirac dark matter annihilates into pairs or triplets of on-shell bosonic mediators to the Standard Model. These annihilation modes allow the dark matter mass to be heavier th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6075c04adc49c79d3dde18f748090504
Publikováno v:
Journal of High Energy Physics. 2013
In the model based on SUSY SU(5) combined with the T' family symmetry, it is shown in Phys. Lett. B 652, 34 (2007) and Phys. Lett. B 681, 444 (2009) that fermion mass hierarchy and mixing angles can be naturally generated in both lepton and quark sec
Publikováno v:
Physical Review D-Particles, Fields, Gravitation and Cosmology, vol 90, iss 1
Physical Review D, vol 90, iss 1
Cotta, RC; Rajaraman, A; Tait, TMP; & Wijangco, AM. (2014). Particle physics implications and constraints on dark matter interpretations of the CDMS signal. Physical Review D-Particles, Fields, Gravitation and Cosmology, 90(1). doi: 10.1103/PhysRevD.90.013020. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/4qh758xx
Physical Review D, vol 90, iss 1
Cotta, RC; Rajaraman, A; Tait, TMP; & Wijangco, AM. (2014). Particle physics implications and constraints on dark matter interpretations of the CDMS signal. Physical Review D-Particles, Fields, Gravitation and Cosmology, 90(1). doi: 10.1103/PhysRevD.90.013020. UC Irvine: Retrieved from: http://www.escholarship.org/uc/item/4qh758xx
Recently the CDMS collaboration has reported an excess of events in the signal region of a search for dark matter scattering with Silicon nuclei. Three events on an expected background of 0.4 have a significance of about 2 sigma, and it is premature
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8b227b74dc049b72e3ef1cc3f27a84d
http://arxiv.org/abs/1305.6609
http://arxiv.org/abs/1305.6609
We derive formulae for neutrino masses and mixing angles in a type I seesaw framework with an underlying A4 flavor symmetry. In particular, the Majorana neutrino mass matrix includes contributions from an A4 triplet, 1, 1', and 1" flavon fields. Usin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38cd9addcb3cf435b608058d426f4972
http://arxiv.org/abs/1210.6982
http://arxiv.org/abs/1210.6982