Evolution of the fine structure constant driven by dark matter and the cosmological constant

نویسندگان
چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Evolution of the Fine Structure Constant Driven by Dark Matter and the Cosmological Constant

Bekenstein’s model of a scalar field, φ, that affects the electromagnetic permeability (usually identified with “changing α”) predicts tiny variations of the effective fine structure constant up to very high red-shifts, |α(z = 3.5)/α0− 1| < 10, when the constraints from Eötvös-Dicke-Braginsky types of experiments are imposed. We generalize this model by allowing additional couplings of φ to bot...

متن کامل

Further evidence for cosmological evolution of the fine structure constant.

We describe the results of a search for time variability of the fine structure constant alpha using absorption systems in the spectra of distant quasars. Three large optical data sets and two 21 cm and mm absorption systems provide four independent samples, spanning approximately 23% to 87% of the age of the universe. Each sample yields a smaller alpha in the past and the optical sample shows a...

متن کامل

Varying Fine-Structure Constant and the Cosmological Constant Problem1

We start with a brief account of the latest analysis of the Oklo phenomenon providing the still most stringent constraint on time-variability of the fine-structure constant α. Comparing this with the recent result from the measurement of distant QSO’s appears to indicate a non-uniform time-dependence, which we argue to be related to another recent finding of the accelerating universe. This view...

متن کامل

A New Cosmological Paradigm: the Cosmological Constant and Dark Matter

The Standard Cosmological Model of the 1980’s is no more. I describe the definitive evidence that the density of matter is insufficient to result in a flat universe, as well as the mounting evidence that the cosmological constant is not zero. I finally discuss the implications of these results for particle physics and direct searches for non-baryonic dark matter, and demonstrate that the new ne...

متن کامل

Supersymmetric dark matter with a cosmological constant

Recent measurements of cosmological parameters from the microwave background radiation, type Ia supernovae, and the age of globular clusters help determine the relic matter density in the universe. It is first shown with mild cosmological assumptions that the relic matter density satisfies ΩMh 2 < 0.6 independent of the cosmological constant and independent of the SNIa data. Including the SNIa ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Physical Review D

سال: 2002

ISSN: 0556-2821,1089-4918

DOI: 10.1103/physrevd.65.085044