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相关论文: Limits on Neutron Lorentz Violation from Pulsar Ti…

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Searches for Lorentz violation were recently extended to the weak sector, in particular neutron and nuclear $\beta$ decay [1]. From experiments on forbidden $\beta$-decay transitions strong limits in the range of $10^{-6}$-$10^{-8}$ were…

高能物理 - 唯象学 · 物理学 2015-03-10 K. K. Vos , H. W. Wilschut , R. G. E. Timmermans

From a cosmological perspective, scalar fields are well-motivated dark matter and dark energy candidates. Several possibilities of neutrino couplings with a time-varying cosmic field have been investigated in the literature. In this work,…

高能物理 - 唯象学 · 物理学 2024-05-02 Rubén Cordero , Luis A. Delgadillo

Pulsar timing, i.e. the analysis of the arrival times of pulses from a pulsar, is a powerful tool in modern astrophysics. It allows us to measure the time delays of an electromagnetic signal caused by a number of physical processes as the…

天体物理仪器与方法 · 物理学 2025-02-04 Konstantin A. Postnov , Nataliya K. Porayko , Maxim S. Pshirkov

Supernova explosions provide the most sensitive probes of neutrino propagation, such as the possibility that neutrino velocities might be affected by the foamy structure of space-time thought to be generated by quantum-gravitational (QG)…

高能物理 - 唯象学 · 物理学 2015-05-30 John Ellis , Hans-Thomas Janka , Nikolaos E. Mavromatos , Alexander S. Sakharov , Edward K. G. Sarkisyan

Working in the context of a Lorentz-violating extension of the standard model we show that estimates of Lorentz symmetry violation extracted from ultra-high energy cosmic rays beyond the Greisen-Kuzmin-Zatsepin (GZK) cutoff allow for…

广义相对论与量子宇宙学 · 物理学 2008-11-26 O. Bertolami , C. S. Carvalho

In this proceedings, I summarize two recently discovered theoretical implications that Lorentz violation has on physical systems. First, I discuss new models for neutrino oscillations in which relatively simple combinations of…

高能物理 - 唯象学 · 物理学 2009-11-10 Don Colladay

Relating the effective Lorentz violation coefficients for composite particles to the coefficients for their constituent fields is a challenging problem. We calculate the Lorentz violation coefficients relevant to the dynamics of an…

高能物理 - 唯象学 · 物理学 2010-01-08 Brett Altschul

The apparent times and positions of moving clocks as predicted by both `non-local' and `local' Lorentz Transformations are considered. Only local transformations respect translational invariance. Such transformations change temporal but not…

综合物理 · 物理学 2011-11-10 J. H. Field

Shear-driven turbulence in the superfluid interior of a neutron star exerts a fluctuating torque on the rigid crust, causing the rotational phase to walk randomly. The phase fluctuation spectrum is calculated analytically for incompressible…

高能天体物理现象 · 物理学 2015-06-17 Andrew Melatos , Bennett Link

We present constraints on violations of Lorentz Invariance based on Lunar Laser Ranging (LLR) data. LLR measures the Earth-Moon separation by timing the round-trip travel of light between the two bodies, and is currently accurate to a few…

广义相对论与量子宇宙学 · 物理学 2008-11-26 James B. R. Battat , John F. Chandler , Christopher W. Stubbs

A general discussion is given of signals for broken Lorentz symmetry in short-baseline neutrino experiments. Among the effects that Lorentz violation can introduce are a dependence on energy differing from that of the usual massive-neutrino…

高能物理 - 唯象学 · 物理学 2008-11-26 Alan Kostelecky , Matthew Mewes

Young pulsars deviate from a perfectly regular spin-down by two non-deterministic phenomena: impulsive glitches and timing noise. Both phenomena are interesting per se, and may provide insights into the superfluid properties of neutron…

高能天体物理现象 · 物理学 2023-02-17 Marco Antonelli , Avishek Basu , Brynmor Haskell

Tests of CPT and Lorentz symmetry using neutral-meson oscillations are studied within a formalism that allows for indirect CPT and T violation of arbitrary size and is independent of phase conventions. The analysis is particularly…

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

Special relativity asserts that physical phenomena appear the same for all inertially moving observers. This symmetry, called Lorentz symmetry, relates long wavelengths to short ones: if the symmetry is exact it implies that spacetime must…

天体物理学 · 物理学 2011-07-19 T. Jacobson , S. Liberati , D. Mattingly

An optical ring cavity is used to place the first laboratory constraints on parity-odd nonrenormalizable Lorentz violation. Variations in resonant frequencies are limited to parts in $10^{15}$. Absolute sensitivity to Lorentz-violating…

广义相对论与量子宇宙学 · 物理学 2013-12-30 Yuta Michimura , Matthew Mewes , Nobuyuki Matsumoto , Yoichi Aso , Masaki Ando

Observations of pulsar glitches may provide insights on the internal physics of neutron stars and recent studies show how it is in principle possible to constrain pulsar masses with timing observations. The reliability of these estimates…

高能天体物理现象 · 物理学 2020-02-12 Alessandro Montoli , Marco Antonelli , Pierre Pizzochero

A relativistic theory for neutrino superluminality is presented (in principle, the same mechanism applies also to other fermions). The theory involves the standard-model particles and one additional heavy sterile neutrino with an…

高能物理 - 唯象学 · 物理学 2017-08-23 F. R. Klinkhamer

A simplified form of a nonsymmetric metric is used to develop the coupling of the electrostatic and gravitational fields, which only occurs in dynamic solutions. The coupling results in a resonance in an object near the Schwarzschild…

天体物理学 · 物理学 2007-05-23 G. Osborn

We consider neutrino oscillations in the minimal Standard-Model Extension describing general Lorentz and CPT violation. Among the models without neutrino mass differences is one with two degrees of freedom that reproduces most major…

高能物理 - 唯象学 · 物理学 2009-07-09 Alan Kostelecky , Matthew Mewes

Millisecond pulsars are intrinsically very stable clocks and precise measurement of their observed pulse periods can be used to study a wide variety of astrophysical phenomena. In particular, observations of a large sample of millisecond…

高能天体物理现象 · 物理学 2015-05-27 R. N. Manchester