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The Peccei-Quinn anomalous global U(1)_{PQ} symmetry is important not only for solving the strong CP problem with a cosmologically relevant axion, but it may also be the origin of a residual Z_2 symmetry. This new symmetry may be…

High Energy Physics - Phenomenology · Physics 2014-03-12 Basudeb Dasgupta , Ernest Ma , Koji Tsumura

Upon embedding the axion-inflation in the minimal left-right symmetric gauge extension of the SM with gauge group $SU(2)_L\times SU(2)_R \times U(1)_{B-L}$, [arXiv:2012.11516] proposed a new particle physics model for inflation. In this…

High Energy Physics - Phenomenology · Physics 2021-10-26 Azadeh Maleknejad

The asymmetric dark matter scenario is known to give an interesting solution for the cosmic coincidence problem between baryon and dark matter densities. In the scenario, the dark matter asymmetry, which is translated to the dark matter…

High Energy Physics - Phenomenology · Physics 2015-05-27 Naoyuki Haba , Shigeki Matsumoto , Ryosuke Sato

SO(10) grand unified theory with minimum parameters in the Yukawa sector employs the Peccei-Quinn symmetry that solves the strong CP problem. Such an economical Yukawa sector is highly appealing and has been extensively studied in the…

High Energy Physics - Phenomenology · Physics 2024-03-08 Ajay Kaladharan , Shaikh Saad

I suggest a new extension of the standard model of particle physics, which introduces a dark sector with the $SU(2)_{D}\otimes U(1)_{D'}$ symmetry besides the SM sector. The new particles of the model all inhabit in the dark sector. The…

High Energy Physics - Phenomenology · Physics 2019-06-26 Wei-Min Yang

We discuss production of QCD axion dark matter in a novel scenario, which assumes time-varying scale of Peccei-Quinn symmetry breaking. The latter decreases as the Universe's temperature at early times and eventually stabilises at a large…

High Energy Physics - Phenomenology · Physics 2023-05-30 Sabir Ramazanov , Rome Samanta

Global symmetries are expected to be violated by gravity, which may cause a serious problem to models based on these symmetries. A famous example is the Peccei-Quinn solution to the strong CP problem in QCD axion models; it requires a…

High Energy Physics - Theory · Physics 2022-04-20 Koichi Hamaguchi , Yoshiki Kanazawa , Natsumi Nagata

Quintessential inflation provides a unified description of inflation and dark energy in terms of a single scalar degree of freedom, the cosmon. We present here a comprehensive overview of this appealing paradigm, highlighting its key…

Cosmology and Nongalactic Astrophysics · Physics 2022-02-04 Dario Bettoni , Javier Rubio

We propose two models where a U(1) Peccei-Quinn global symmetry arises accidentally and is respected up to high-dimensional operators, so that the axion solution to the strong CP problem is successful even in the presence of…

High Energy Physics - Phenomenology · Physics 2021-01-20 Marco Ardu , Luca Di Luzio , Giacomo Landini , Alessandro Strumia , Daniele Teresi , Jin-Wei Wang

To address five fundamental shortcomings of the Standard Model (SM) of particle physics and cosmology, we propose a SMART U(1)$_X$ model which is a $U(1)_X \times U(1)_{PQ}$ extension of the SM. The $U(1)_X$ gauge symmetry is a…

High Energy Physics - Phenomenology · Physics 2020-12-02 Nobuchika Okada , Digesh Raut , Qaisar Shafi

We propose a non-universal $\mathrm{U}(1)_{X}$ gauge extension to the Standard Model (SM) and an additional Peccei-Quinn (PQ) global symmetry to study the mass hierarchy and strong CP problem. The scheme allows us to distinguish among…

High Energy Physics - Phenomenology · Physics 2021-05-18 Y. A. Garnica , S. F. Mantilla , R. Martinez , H. Vargas

We propose a scenario of brane cosmology in which the Peccei-Quinn field plays the role of the inflaton and solves simultaneously many cosmological and phenomenological issues such as the generation of a heavy Majorana mass for the…

High Energy Physics - Phenomenology · Physics 2016-05-16 Gabriela Barenboim , Wan-Il Park

The main limitation for preinflationary breaking of Peccei-Quinn (PQ) symmetry is the upper bound on the Hubble rate during inflation from axion isocurvature fluctuations. This leads to a tension between high scale inflation and QCD axions…

High Energy Physics - Phenomenology · Physics 2024-11-13 Maximilian Berbig

I suggest an extension of the SM by introducing a dark sector with the local $U(1)_{D}$ symmetry. The particles in the dark sector bring about the new physics beyond the SM. In particular the global $B-L$ symmetry is violated just above the…

High Energy Physics - Phenomenology · Physics 2017-08-25 Wei-Min Yang

A moderate extension of the minimal supersymmetric standard model which includes a U(1)_(B-L) gauge group (B and L being the baryon and lepton number) and a Peccei-Quinn symmetry, U(1)_PQ, is presented. The hybrid inflationary scenario is…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides

We construct the New Minimal Standard Model that incorporates the new discoveries of physics beyond the Minimal Standard Model (MSM): Dark Energy, non-baryonic Dark Matter, neutrino masses, as well as baryon asymmetry and cosmic inflation,…

High Energy Physics - Phenomenology · Physics 2009-09-29 Hooman Davoudiasl , Ryuichiro Kitano , Tianjun Li , Hitoshi Murayama

The companion-axion model introduces a second QCD axion to rescue the Peccei-Quinn solution to the strong-CP problem from the effects of colored gravitational instantons. As in single-axion models, the two axions predicted by the…

High Energy Physics - Phenomenology · Physics 2025-06-18 Zhe Chen , Archil Kobakhidze , Ciaran A. J. O'Hare , Zachary S. C. Picker , Giovanni Pierobon

In the early Universe, any particle carrying a conserved quantum number and in chemical equilibrium with the thermal bath will unavoidably inherit a particle-antiparticle asymmetry. A new particle of this type, if stable, would represent a…

High Energy Physics - Phenomenology · Physics 2015-07-08 Sofiane M. Boucenna , Martin B. Krauss , Enrico Nardi

We propose a novel framework for low-scale leptogenesis within an extension of the Standard Model (SM) that includes three SU(2) singlet right-handed neutrinos, a singlet charged neutral fermion, and a real scalar field. In this setup, the…

High Energy Physics - Phenomenology · Physics 2026-01-01 Suresh Chand , Avnish , Poulose Poulose

We introduce a minimal and yet comprehensive framework with $CP$- and classical scale-symmetries, in order to simultaneously address the hierarchy problem, neutrino masses, dark matter, and inflation. One complex gauge singlet scalar and…

High Energy Physics - Phenomenology · Physics 2016-04-20 Arsham Farzinnia , Seyen Kouwn