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We study the CP domain walls and the consequent gravitational waves induced by the spontaneous breaking of the CP symmetry in the complex singlet extension to the Standard Model. We impose the constraints from the unitarity, stability and…

高能物理 - 唯象学 · 物理学 2020-04-22 Ning Chen , Tong Li , Yongcheng Wu

Here we briefly review possible indirect effects of dark matter (DM) of the Universe. It includes effects in cosmic rays (CR): first of all, the positron excess at $\sim$ 500 GeV and possible electron-positron excess at 1-1.5 TeV. We tell…

高能物理 - 唯象学 · 物理学 2019-12-12 K. M. Belotsky , E. A. Esipova , A. Kh. Kamaletdinov , E. S. Shlepkina , M. L. Solovyov

Motivated by a recent detection of 511 keV photons from the center of our Galaxy, we calculate the spectrum of the soft gamma-ray background of the redshifted 511 keV photons from cosmological halos. Annihilation of dark matter particles…

天体物理学 · 物理学 2009-11-10 Kyungjin Ahn , Eiichiro Komatsu

Geometric phases can manifest when a relativistic quantum particle moves cyclically along a loop in parameter space. The phase can be affected by the presence of a background field and can be accompanied by nontrivial topological features.…

高能物理 - 唯象学 · 物理学 2025-12-02 Alan Kostelecky , Ralf Lehnert , Marco Schreck , Babak Seradjeh

The parameter epsilon_K, that quantifies CP violation in kaon mixing, is the observable setting the strongest constraints on new physics with a generic flavour and CP structure. While its experimental uncertainty is at the half percent…

高能物理 - 唯象学 · 物理学 2016-06-03 Filippo Sala

We propose methods for extracting limits on the strength of P-odd interactions of pseudoscalar and pseudovector cosmic fields with electrons, protons and neutrons. Candidates for such fields are dark matter (including axions) and dark…

高能物理 - 唯象学 · 物理学 2014-08-21 B. M. Roberts , Y. V. Stadnik , V. A. Dzuba , V. V. Flambaum , N. Leefer , D. Budker

We consider the case of a coupling in the dark cosmological sector, where a dark energy scalar field modifies the gravitational attraction between dark matter particles. We find that the strength of the coupling {\beta} is constrained using…

宇宙学与河外天体物理 · 物理学 2013-05-30 Valeria Pettorino , Luca Amendola , Carlo Baccigalupi , Claudia Quercellini

We perform observational confrontation and cosmographic analysis of $f(T,T_G)$ gravity and cosmology. This higher-order torsional gravity is based on both the torsion scalar, as well as on the teleparallel equivalent of the Gauss--Bonnet…

广义相对论与量子宇宙学 · 物理学 2024-10-15 Harshna Balhara , J. K. Singh , Shaily , Emmanuel N. Saridakis

The strong CP-violating parameter is small today as indicated by constraints on the neutron electric dipole moment. In the early universe, the QCD axion has not yet relaxed to its QCD-cancelling minimum and it is natural to wonder whether…

高能物理 - 唯象学 · 物理学 2014-10-29 Geraldine Servant

In this paper we show that the baryon-to-photon ratio $\eta$ is in general not conserved before decoupling in non-minimally coupled theories of gravity. We use big-bang nucleosynthesis and cosmic microwave background limits on the…

广义相对论与量子宇宙学 · 物理学 2018-10-03 R. P. L. Azevedo , P. P. Avelino

The expectation values of energy density and pressure of a quantum field inside a wedge-shaped region appear to violate the expected relationship between torque and total energy as a function of angle. In particular, this is true of the…

高能物理 - 理论 · 物理学 2013-03-07 S. A. Fulling , F. D. Mera , C. S. Trendafilova

Light dark matter with sub-eV masses has a high number density in our galaxy, and its scattering cross section with macroscopic objects can be significantly enhanced by coherence effects. Repeated scattering with a target object can induce…

高能物理 - 唯象学 · 物理学 2026-03-31 Shigeki Matsumoto , Jie Sheng , Chuan-Yang Xing , Lin Zhu

The constraints on departures from general relativity (GR) at cosmological length scales due to cosmic microwave background (CMB) data are discussed. The departure from GR is measured by the ratio, parameterized as $1 +\varpi_0 (1 +…

宇宙学与河外天体物理 · 物理学 2009-10-29 Paolo Serra , Asantha Cooray , Scott F. Daniel , Robert Caldwell , Alessandro Melchiorri

In Lorentz- and CPT-violating effective field theories involving scalar and spinor fields, there exist forms of Lorentz violation that modify only the scalar-spinor Yukawa interaction vertices. These affect low-energy fermion and…

高能物理 - 理论 · 物理学 2013-05-21 Brett Altschul

We propose an experimental test of the gravitational interaction with antimatter by measuring the branching fraction of the CP~violating decay $K_\mathrm{L} \to \pi^{+} \pi^{-}$ in space. We show that at the altitude of the International…

高能物理 - 唯象学 · 物理学 2016-05-09 Giovanni Maria Piacentino , Anthony Palladino , Graziano Venanzoni

We report here the results of operation of a torsion balance with a period of $\sim 1.27 \times 10^4$ s. The analysis of data collected over a period of $\sim$115 days shows that the difference in the accelerations towards the Galactic…

Infrared, optical, and ultraviolet spectropolarimetry of cosmological sources is used to constrain the pure electromagnetic sector of a general Lorentz-violating standard-model extension. The coefficients for Lorentz violation are bounded…

高能物理 - 唯象学 · 物理学 2009-09-25 Alan Kostelecky , Matthew Mewes

We use fits to recent published CPLEAR data on neutral kaon decays to $\pi^+\pi^-$ and $\pi e\nu$ to constrain the CPT--violation parameters appearing in a formulation of the neutral kaon system as an open quantum-mechanical system. The…

高能物理 - 实验 · 物理学 2008-11-26 R. Adler , etal , J. Ellis , J. Lopez , N. Mavromatos , D. Nanopoulos

We study CMB constraints on a model with a cosmological constant and a fraction of dark matter non-minimally coupled to a massless scalar field. In this scenario, there is an extra gravity-like fifth force which can affect the evolution of…

宇宙学与河外天体物理 · 物理学 2018-05-09 Sophie C. F. Morris , Anne M. Green

CP violation due to interference between $K_L$ and $K_S$ decays into $\pi ^+\pi^-\gamma$ is analyzed in the Standard Model. The CP-violating parameter $\epsilon'_{+- \gamma}$, which is the difference between $\eta_{+-\gamma}$ and…

高能物理 - 唯象学 · 物理学 2010-11-01 Hai-Yang Cheng
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