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相关论文: Cosmological chirality and magnetic fields from pa…

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We argue that the presence of a very strong magnetic field in the chirally broken phase induces inhomogeneous expectation values, of a spiral nature along the magnetic field axis, for the currents of charge and chirality, when there is…

高能物理 - 唯象学 · 物理学 2010-11-11 Gokce Basar , Gerald V. Dunne , Dmitri E. Kharzeev

We propose a way to introduce the currents responsible for the Chiral Magnetic Effect, and similar phenomena, into the AdS/CFT description. Such currents are thought to occur in heavy ion collisions due to topologically non-trivial field…

高能物理 - 理论 · 物理学 2011-07-08 Lionel Brits , James Charbonneau

We show that a parity-breaking uniform (averaged over all directions on the sky) circular polarization of amplitude $V_{00} \simeq 2.6 \times 10^{-17}\, \Delta \chi (r/0.06)$ can be induced by chiral gravitational-wave (GW) background with…

宇宙学与河外天体物理 · 物理学 2019-07-26 Keisuke Inomata , Marc Kamionkowski

Large magnetic fields exist in magnetars and are produced in off-central heavy-ion collisions. For the latter, field strengths are estimated to be comparable to strong interaction scales. This fact has motivated many studies of QCD physics…

高能物理 - 唯象学 · 物理学 2024-08-20 Prabal Adhikari , Brian C. Tiburzi

The causality principle imposes the constraints on the cosmological parameters in the relativistic theory of gravitation. As a result, X-matter causes the quite definite cosmological scenario with the alternate acceleration and deceleration…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. L. Kalashnikov

A chiral chemical potential present in the early universe can source helical hypermagnetic fields through the chiral plasma instability. If these hypermagnetic fields survive until the electroweak phase transition, they source a…

高能物理 - 唯象学 · 物理学 2023-07-12 Valerie Domcke , Kohei Kamada , Kyohei Mukaida , Kai Schmitz , Masaki Yamada

Many particle physics models of matter admit solutions corresponding to stable or long-lived topological defects. In the context of standard cosmology it is then unavoidable that such defects will form during phase transitions in the very…

高能物理 - 唯象学 · 物理学 2009-10-31 Robert H. Brandenberger

At finite density parity can be spontaneously broken in strong interactions with far reaching implications. In particular, a time-dependent pseudoscalar background would modify QED by adding a Chern-Simons term to the lagrangian. As a…

高能物理 - 唯象学 · 物理学 2011-09-21 Alexander Andrianov , Vladimir Andrianov , Domenec Espriu , Xumeu Planells

Some solutions of the hierarchy problem of particle physics can lead to significantly increased neutrino cross sections beyond the electroweak scale. We discuss some consequences for and constraints resulting from cosmic ray physics.

高能物理 - 唯象学 · 物理学 2009-10-31 Guenter Sigl

The chiral magnetic effect (CME) refers to charge separation along a strong magnetic field of single-handed quarks, caused by interactions with topological gluon fields from QCD vacuum fluctuations. A major background of CME measurements in…

核实验 · 物理学 2018-05-08 Jie Zhao

The origin of the substantial magnetic fields that are found in galaxies and on even larger scales, such as in clusters of galaxies, is yet unclear. If the second-order couplings between photons and electrons are considered, then…

天体物理学 · 物理学 2007-05-23 Kiyotomo Ichiki , Keitaro Takahashi , Hiroshi Ohno , Hidekazu Hanayama , Naoshi Sugiyama

A comparison of the standard models in particle physics and in cosmology demonstrates that they are not compatible, though both are well established. Basics of modern cosmology are briefly reviewed. It is argued that the measurements of the…

高能物理 - 唯象学 · 物理学 2008-11-26 A. D. Dolgov

The peculiar motion of an observer with respect to the CMB rest frame induces an apparent deflection of the observed CMB photons, {\it i.e.} aberration, and a shift in their frequency, {\it i.e.} Doppler effect. Both effects distort the…

宇宙学与河外天体物理 · 物理学 2015-06-11 Riccardo Catena , Alessio Notari

The claim by Gurzadyan et al. that the cosmological sky is a weakly random one where "the random perturbation is a minor component of mostly regular signal" has given rise to a series of useful exchanges. The possibility that the Cosmic…

综合物理 · 物理学 2011-10-31 Luis Gonzalez-Mestres

We propose that cosmological magnetic fields generated in regions of finite spatial dimensions may manifest themselves in the global dynamics of the Universe as `dark energy'. We test our model in the context of spatially flat cosmological…

天体物理学 · 物理学 2019-08-19 Ioannis Contopoulos , Spyros Basilakos

The long-standing anomaly in the anomalous magnetic moment of the muon indicates the presence of chirality violating new physics contributions. A possible solution involves scalar leptoquarks with left- and right-handed couplings to the top…

高能物理 - 唯象学 · 物理学 2017-03-29 Estefania Coluccio Leskow , Andreas Crivellin , Giancarlo D'Ambrosio , Dario Müller

The effects of chiral imbalance and external magnetic field on pion superfluidity and color superconductivity are investigated in extended Nambu--Jona-Lasinio models. We take Schwinger approach to treat the interaction between charged pion…

核理论 · 物理学 2016-01-22 Gaoqing Cao , Pengfei Zhuang

By completing the old discussion of K.~Wilson, we express the chiral anomaly in terms of a double integral of a three-point function of chiral currents over an arbitrarily small region in the coordinate space. An integrability condition…

高能物理 - 理论 · 物理学 2016-08-24 Hidenori Sonoda

The chiral magnetic effect (CME) is an exact statement that connects via the axial anomaly the electric current in a system consisting of interacting fermions and gauge field with chirality imbalance that is put into a strong external…

高能物理 - 唯象学 · 物理学 2020-04-17 L. Ya. Glozman

We compute (pseudo)critical temperature, $T_c$, of chiral symmetry restoration for quark matter in the background of parallel electric and magnetic fields. This field configuration leads to the production of a chiral medium on a time scale…

高能物理 - 唯象学 · 物理学 2016-12-21 Marco Ruggieri , Guang Xiong Peng , Maxim Chernodub