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相关论文: Peccei-Quinn Relaxion

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The dynamical relaxation provides an interesting solution to the hierarchy problem in face of the missing signatures of any new physics in recent experiments. Through a dynamical process taking place in the inflationary phase of the…

高能物理 - 唯象学 · 物理学 2018-02-21 Zygmunt Lalak , Adam Markiewicz

Solutions to the strong CP problem typically introduce new scales associated with the spontaneous breaking of symmetries. Absent any anthropic argument for small $\bar\theta$, these scales require stabilization against ultraviolet…

高能物理 - 唯象学 · 物理学 2016-01-27 Abdelhamid Albaid , Michael Dine , Patrick Draper

The Higgs naturalness problem is solved if the growth of Einstein's gravitational interaction is softened at an energy $ \lesssim 10^{11}\,$GeV (softened gravity). We work here within an explicit realization where the Einstein-Hilbert…

高能物理 - 唯象学 · 物理学 2017-06-23 Alberto Salvio

Slightly extending a right-handed neutrino version of the $3-3-1$ model, we show that it is not only possible to solve the strong CP problem but also to give the total dark matter abundance reported by the Planck collaboration.…

高能物理 - 唯象学 · 物理学 2018-04-13 J. C. Montero , Ana R. Romero Castellanos , B. L. Sánchez-Vega

Observable primordial tensor modes in the cosmic microwave background (CMB) would point to a high scale of inflation $H_{I}$. If the scale of Peccei-Quinn (PQ) breaking $f_a$ is greater than $\frac{H_{I}}{2\pi}$, CMB constraints on…

高能物理 - 唯象学 · 物理学 2016-06-07 John Kearney , Nicholas Orlofsky , Aaron Pierce

Peccei-Quinn (PQ) mechanism based on a chiral global U(1) symmetry is considered to be a simple and elegant solution for strong CP problem. Fact that the mechanism could be experimentally examined through the axion search makes it much more…

高能物理 - 唯象学 · 物理学 2018-11-14 Daijiro Suematsu

We examine the sensitivity of several solutions of the strong-CP problem to violations of global symmetries by Planck scale physics. We find that the Peccei-Quinn solution is extremely sensitive to U(1)_PQ violating operators of dimension…

高能物理 - 唯象学 · 物理学 2010-11-01 R. Holman , S. D. H. Hsu , T. Kephart , E. Kolb , R. Watkins , L. Widrow

In light of no discovered new physics at the LHC, ideas which tackle the Hierarchy Problem without novelties around the TeV scale must be taken seriously. Such is a cosmological relaxation model of the Higgs mass, proposed in the pre-LHC…

高能物理 - 唯象学 · 物理学 2020-07-29 Marco Michel

It is firmly believed that the axion for solving the strong CP problem must come from the spontaneous breaking of an anomalous Peccei-Quinn global symmetry. Here we show a new possibility that the axion can be induced by a pseudo Goldstone…

高能物理 - 唯象学 · 物理学 2023-07-11 Pei-Hong Gu

We suggest that the electroweak Higgs particles can be identified with extra-dimensional components of the gauge fields, which after compactification on a certain topologically non-trivial background become tachyonic and condense. If the…

高能物理 - 唯象学 · 物理学 2009-11-07 G. Dvali , S. Randjbar-Daemi , R. Tabbash

Considerable theoretical efforts have gone into expanding the reach of the QCD axion beyond its canonical mass--decay-constant relation. The $Z_\mathcal{N}$ QCD axion model reduces the QCD axion mass naturally, by invoking a discrete…

高能物理 - 唯象学 · 物理学 2026-02-24 Raymond T. Co , Taegyu Lee , Owen P. Leonard

We argue that the QCD axion can arise from many aligned axions with decay constants much smaller than the conventional axion window. If the typical decay constant is of {\cal O}{(100)} GeV to 1 TeV, one or more of the axions or saxions may…

高能物理 - 唯象学 · 物理学 2016-02-03 Tetsutaro Higaki , Kwang Sik Jeong , Naoya Kitajima , Fuminobu Takahashi

We explore a simple model which naturally explains the observed baryon asymmetry of the Universe. In this model the strong coupling is promoted to a dynamical quantity, which evolves through the vacuum expectation value of a singlet scalar…

高能物理 - 唯象学 · 物理学 2020-04-08 Djuna Croon , Jessica N. Howard , Seyda Ipek , Timothy M. P. Tait

Inspired by the possibility of high-scale supersymmetry breaking in the string landscape where the cosmological constant problem and the gauge hierarchy problem can be solved while the strong CP problem is still a challenge for naturalness,…

高能物理 - 唯象学 · 物理学 2009-09-15 V. Barger , Cheng-Wei Chiang , Jing Jiang , Tianjun Li

The axion solution to the strong CP problem makes use of a global Peccei-Quinn U(1) symmetry which is susceptible to violations from quantum gravitational effects. We show how discrete gauge symmetries can protect the axion from such…

高能物理 - 唯象学 · 物理学 2010-04-05 K. S. Babu , Ilia Gogoladze , Kai Wang

We present a minimal cosmological solution to the hierarchy problem. Our model consists of a light pseudoscalar and an extra Higgs doublet in addition to the field content of the Standard Model. We consider a landscape of vacua with varying…

高能物理 - 唯象学 · 物理学 2024-07-24 Susobhan Chattopadhyay , Dibya S. Chattopadhyay , Rick S. Gupta

We study the parameter space of cold dark matter axions in two cosmological scenarios with non-standard thermal histories before Big Bang nucleosynthesis: the Low Temperature Reheating (LTR) cosmology and the kination cosmology. If the…

宇宙学与河外天体物理 · 物理学 2021-12-14 Luca Visinelli , Paolo Gondolo

We present global fits of cosmologically stable axion-like particle and QCD axion models in the mass range 0.1 neV to 10 eV. We focus on the case where the Peccei-Quinn symmetry is broken before the end of inflation, such that the initial…

高能物理 - 唯象学 · 物理学 2020-08-19 Sebastian Hoof , Felix Kahlhoefer , Pat Scott , Christoph Weniger , Martin White

Three possible strategies have been advocated to solve the strong CP problem. The first is the axion, a dynamical mechanism that relaxes any initial value of the CP violating angle $\bar{\theta}$ to zero. The second is the imposition of new…

高能物理 - 唯象学 · 物理学 2025-05-14 David E. Kaplan , Tom Melia , Surjeet Rajendran

The discovery of the Higgs particle at around 126 GeV has given us a big hint towards the origin of the Higgs potential. The running quartic self-coupling decreases and crosses zero somewhere in the very high energy scale. It is usually…

高能物理 - 唯象学 · 物理学 2017-08-23 Satoshi Iso
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