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The detection of GW170817 is revolutionizing many areas of astrophysics with the joint observation of gravitational waves and electromagnetic emissions. These multi-messenger events provide a new approach to determine the Hubble constant,…

We present new light curves covering 14 to 19 years of observations of four bright proto-planetary nebulae (PPNs), all O-rich and of F spectral type. They each display cyclical light curves with significant variations in amplitude. All four…

太阳与恒星天体物理 · 物理学 2016-10-26 Bruce J. Hrivnak , Wenxian Lu , Kristie A. Nault

The ultimate fate of the universe, infinite expansion or a big crunch, can be determined by measuring the redshifts, apparent brightnesses, and intrinsic luminosities of very distant supernovae. Recent developments have provided tools that…

Gamma-ray bursts (GRBs) are the most luminous explosions and can be detectable out to the edge of Universe. It has long been thought they can extend the Hubble diagram to very high redshifts. Several correlations between temporal or…

高能天体物理现象 · 物理学 2022-01-26 F. Y. Wang , J. P. Hu , G. Q. Zhang , Z. G. Dai

Progressive increases in the precision of the Hubble-constant measurement via Cepheid-calibrated Type Ia supernovae (SNe Ia) have shown a discrepancy of $\sim 4.4\sigma$ with the current value inferred from Planck satellite measurements of…

宇宙学与河外天体物理 · 物理学 2020-07-01 T. de Jaeger , B. E. Stahl , W. Zheng , A. V. Filippenko , A. G. Riess , L. Galbany

In the conventional / most studied local distance ladder measurements, Type Ia supernovae (SNe Ia) are used in two of the three rungs. In the second rung, their luminosities are calibrated by standard candles like Cepheids or Tip of the Red…

宇宙学与河外天体物理 · 物理学 2023-11-29 Daniel Scolnic , Maria Vincenzi

For spectroscopically confirmed Type Ia supernovae we evaluate models of intrinsic brightness variations with detailed data/Monte Carlo comparisons of the dispersion in the following quantities: Hubble-diagram scatter, color difference…

Hubble tension is one of the most important problems in cosmology. Although the local measurements on the Hubble constant with Type Ia supernovae (SNe Ia) are independent of cosmological models, they suffer the problem of zero-point…

广义相对论与量子宇宙学 · 物理学 2023-10-24 Xuchen Lu , Yungui Gong

Type Ia supernovae (SNe Ia) can be calibrated to be good standard candles at cosmological distances. We propose a supernova pencil beam survey that could yield between dozens to hundreds of SNe Ia in redshift bins of 0.1 up to $z=1.5$,…

天体物理学 · 物理学 2009-10-30 Yun Wang

We present a new model-independent method to determine the spatial curvature and to mitigate the circularity problem affecting the use of quasars as distance indicators. The cosmic-chronometer measurements are used to construct the…

宇宙学与河外天体物理 · 物理学 2020-01-29 Jun-Jie Wei , Fulvio Melia

In this note, we consider the observational constraints on some cosmological models by using the 307 Union type Ia supernovae (SNIa), the 32 calibrated Gamma-Ray Bursts (GRBs) at $z>1.4$, the updated shift parameter $R$ from WMAP 5-year…

天体物理学 · 物理学 2009-03-23 Hao Wei

Type Ia Supernovae are standard candles so their mean apparent magnitude has been exploited to learn about the redshift-distance relationship. Besides intrinsic scatter in this standard candle, additional source of scatter is caused by…

天体物理学 · 物理学 2008-11-26 Scott Dodelson , Alberto Vallinotto

The use of Type~Ia SNe has thus far produced the most reliable measurement of the expansion history of the Universe, suggesting that $\Lambda$CDM offers the best explanation for the redshift--luminosity distribution observed in these…

宇宙学与河外天体物理 · 物理学 2018-06-22 Jun-Jie Wei , Xue-Feng Wu , Fulvio Melia , Robert S. Maier

One of the topical problems of contemporary physics is a possible variability of the fundamental constants. Here we consider possible variability of two dimensionless constants which are most important for calculation of atomic and…

原子物理 · 物理学 2016-09-08 D. A. Varshalovich , A. Y. Potekhin , A. V. Ivanchik

Thermonuclear (Type Ia) supernovae are bright stellar explosions, the light curves of which can be calibrated to allow for use as "standard candles" for measuring cosmological distances. Contemporary research investigates how the brightness…

太阳与恒星天体物理 · 物理学 2017-06-28 Alan C. Calder , Brendan K. Krueger , Aaron P. Jackson , Don E. Willcox , Broxton J. Miles , Dean M. Townsley

Improving the use of Type Ia supernovae (SNIa) as standard candles requires a better approach to incorporate the relationship between SNIa and the properties of their host galaxies. Using a spectroscopically-confirmed sample of $\sim$1600…

宇宙学与河外天体物理 · 物理学 2021-06-02 Brodie Popovic , Dillon Brout , Richard Kessler , Dan Scolnic , Lisa Lu

We have shown that the varying physical constant model is consistent with the recently published variational approach wherein Einstein equations are modified to include the variation of the speed of light c, gravitational constant G and…

宇宙学与河外天体物理 · 物理学 2020-09-21 Rajendra P. Gupta

Motivated by the idea of using quasars as standardizable candles for cosmology, we examine the relation between X-ray (at 2 keV, $L_{\rm 2keV}$) and ultraviolet (at 2500 Angstrom, $L_{\rm 2500}$) monochromatic luminosities of quasars using…

The Hubble's constant is usually surmised to be a constant; but the experiments show a large spread and conflicting estimates. According to the plasma-redshift theory, the Hubble's constant varies with the plasma densities along the line of…

天体物理学 · 物理学 2007-05-23 Ari Brynjolfsson