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Recent progress in cosmic ray physics covering the energy range from about 10^{14} eV to 10^{19} eV is reviewed. The most prominent features of the energy spectrum are the so called `knee' at E ~ 3 * 10^{15} eV and the `ankle' at few…

天体物理学 · 物理学 2008-11-26 Karl-Heinz Kampert

We discuss a possible answer to the fundamental question of why nature would actually prefer low-scale supersymmetry, but end up with a supersymmetry scale that is not completely natural. This question is inevitable if we postulate that…

高能物理 - 唯象学 · 物理学 2015-09-30 Keisuke Harigaya , Masahiro Ibe , Kai Schmitz , Tsutomu T. Yanagida

Most of the calculations done to obtain the value of the cosmological constant use methods of quantum gravity, a theory that has not been established as yet, and a variety of results are usually obtained. The numerical value of the…

天体物理学 · 物理学 2007-05-23 Moshe Carmeli

Atomic and molecular electric dipole moments are calculated within the minimal supersymmetric standard model. Present experiments already provide strong bounds on the combination of phases responsible for the dipole moments of the neutron…

高能物理 - 唯象学 · 物理学 2010-11-01 Willy Fischler , Sonia Paban , Scott Thomas

Within present constraints on the observed smooth energy and its equation of state parameter, it is important to find out whether the smooth energy is static (cosmological constant) or dynamic (quintessence). The most dynamical quintessence…

天体物理学 · 物理学 2009-04-13 S. A. Bludman , M. Roos

Our knowledge of the mass composition of cosmic rays is deficient at all energies above 10^17. Here systematic differences between different measurements are discussed and, in particular, it is argued that there is no compelling evidence to…

天体物理学 · 物理学 2009-11-10 A. A. Watson

A general-relativistic theory of cosmology, the dynamical variables of which are those of Hubble's, namely distances and redshifts, is presented. The theory describes the universe as having a three-phase evolution with a decelerating…

天体物理学 · 物理学 2007-05-23 S. Behar , M. Carmeli

We investigate whether a mass scale for elementary particles can be derived from interactions of particles with distant matter in the Universe, the mechanism of the interaction being the classical vector potential, propagating in a space of…

广义相对论与量子宇宙学 · 物理学 2007-07-31 Peter R. Phillips

This review summarizes recent developments in the understanding of high-energy cosmic rays. It focuses on galactic and presumably extragalactic particles in the energy range from the knee (10^15 eV) up to the highest energies observed…

高能天体物理现象 · 物理学 2009-10-06 J. Bluemer , R. Engel , J. R. Hoerandel

Measurements of cosmic ray particles at energies above E = 5 x 10^{14} eV are performed by large area ground based air shower experiments. Only they provide the collection power required for obtaining sufficient statistics at the low flux…

天体物理学 · 物理学 2008-11-26 Karl-Heinz Kampert

A new measurement of the cosmic ray positron fraction in the energy range of 1-50 GeV is presented. The measurement is based on data taken by the AMS-01 experiment during its 10 day space shuttle flight in June 1998. A proton background…

天体物理学 · 物理学 2007-05-23 Henning Gast , Jan Olzem , Stefan Schael

Vacuum energy changes during cosmological phase transitions and becomes relatively important at epochs just before phase transitions. For a viable cosmology the vacuum energy just after a phase transition must be set by the critical…

宇宙学与河外天体物理 · 物理学 2016-07-20 Brando Bellazzini , Csaba Csaki , Jay Hubisz , Javi Serra , John Terning

Although supersymmetry has not been seen directly by experiment, there are powerful physics reasons to suspect that it should be an ingredient of nature and that superpartner masses should be somewhat near the weak scale. I present an…

高能物理 - 唯象学 · 物理学 2009-11-10 James D. Wells

The SKA will build upon early detections of the EoR by precursor instruments, such as MWA, PAPER, and LOFAR, and planned instruments, such as HERA, to make the first high signal-to-noise measurements of fluctuations in the 21 cm brightness…

We have proposed that the cosmic ray spectrum "knee", the steepening of the cosmic ray spectrum at energy $E \gsim 10^{15.5}$ eV, is due to "new physics", namely new interactions at TeV cm energies which produce particles undetected by the…

高能物理 - 唯象学 · 物理学 2015-06-25 D. Kazanas , A. Nicolaidis

Power-law cosmology with scale factor as power of cosmic time, $a \propto t^{\a}$, is investigated. We review and discuss value of $\a$ obtained from various types of observation. Considering dark energy dominant era in late universe from…

宇宙学与河外天体物理 · 物理学 2013-08-30 Burin Gumjudpai

I briefly review cosmological bounds on neutrino masses and the underlying gravitational physics at a level appropriate for readers outside the field of cosmology. For the case of three massive neutrinos with standard model freezeout, the…

高能物理 - 唯象学 · 物理学 2009-10-07 Max Tegmark

This is a review article for The Review of Particle Physics 2026 (aka the Particle Data Book), appearing as Chapter 25. It forms a compact review of knowledge of the cosmological parameters near the end of 2025. Topics included are…

宇宙学与河外天体物理 · 物理学 2026-02-17 Marina Cortês , Ofer Lahav , Andrew R Liddle

Recently, a model for an emergent gravity based on $SO(5)$ Yang-Mills action in Euclidian 4-dimensional spacetime was proposed. In this work we provide some 1 and 2-loops computations and show that the model can accommodate suitable…

高能物理 - 理论 · 物理学 2016-09-15 Rodrigo F. Sobreiro , Anderson A. Tomaz

The spectrum of ultrahigh energy (above \approx 10^{9} GeV) cosmic rays is consistent with the decay of GUT scale particles. The predicted mass is m_X=10^b GeV, where b=14.6_{-1.7}^{+1.6}.

高能物理 - 唯象学 · 物理学 2009-10-31 Z. Fodor , S. D. Katz