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相关论文: Measuring dark energy with the $E_{\rm iso}-E_{\rm…

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We update gamma-ray burst (GRB) luminosity relations among certain spectral and light-curve features with 139 GRBs. The distance modulus of 82 GRBs at $z>1.4$ can be calibrated with the sample at $z\leq1.4$ by using the cubic spline…

宇宙学与河外天体物理 · 物理学 2015-09-23 Jun-Jie Wei , Qing-Bo Ma , Xue-Feng Wu

In this paper we analyze the constraints on the property of dark energy from cosmological observations. Together with SNe Ia Gold sample, WMAP, SDSS and 2dFGRS data, we include 69 long Gamma-Ray Bursts (GRBs) data in our study and perform…

天体物理学 · 物理学 2008-11-26 Hong Li , Meng Su , Zuhui Fan , Zigao Dai , Xinmin Zhang

Recently, both theoretical arguments and observational evidence suggested that a small fraction of fast radio bursts (FRBs) could be associated with gamma-ray bursts (GRBs). If such FRB/GRB association systems are commonly detected in the…

宇宙学与河外天体物理 · 物理学 2015-06-18 He Gao , Zhuo Li , Bing Zhang

We report results of a systematic study of the broad band (2--2000 keV) time resolved prompt emission spectra of a sample of gamma-ray bursts (GRBs) detected with both Wide Field Cameras on board the \sax\ satellite and the \batse\…

高能天体物理现象 · 物理学 2015-06-05 Filippo Frontera , Lorenzo Amati , Cristiano Guidorzi , Raffaella Landi , Jean in't Zand

We extend the Hubble diagram up to $z = 5.6$ using 63 gamma-ray bursts (GRBs) via peak energy-peak luminosity relation (so called Yonetoku relation), and obtain constraints on cosmological parameters including dynamical dark energy…

From a comprehensive statistical analysis of $Swift$ X-ray light-curves of gamma-ray bursts (GRBs) collected from December 2004 to the end of 2010, we found a three-parameter correlation between the isotropic energy emitted in the rest…

高能天体物理现象 · 物理学 2015-11-18 Elena Zaninoni , Maria Grazia Bernardini , Raffaella Margutti , Lorenzo Amati

In this paper, we examine the spacial distribution of gamma-ray bursts (GRBs) using a sample of 373 objects. We subdivide the GRB data into two redshift intervals over the redshift range $0<z< 6.7$. We measure the two-point correlation…

宇宙学与河外天体物理 · 物理学 2015-07-07 Ming-Hua Li , Hai-Nan Lin

In this paper, we compile a \emph{Fermi} sample of the \emph{long} GRB observations from 15 years of GBM catalogue with identified redshift, in which the GOLD sample contains 123 long GRBs at $z\le5.6$ and the FULL sample contains 151 long…

宇宙学与河外天体物理 · 物理学 2025-04-04 Huifeng Wang , Nan Liang

Gamma-ray bursts (GRBs) are ultra-relativistic collimated outflows, which emit synchrotron radiation throughout the entire electromagnetic spectrum when they interact with their environment. This afterglow emission enables us to probe the…

高能天体物理现象 · 物理学 2022-02-09 M. D. Aksulu , R. A. M. J. Wijers , H. J. van Eerten , A. J. van der Horst

The correlations between the rest frame peak of the EF_E spectrum of GRBs Epeak and their isotropic energy (E_iso) or luminosity (L_iso) could have several implications for the understanding of the GRB prompt emission. These correlations…

高能天体物理现象 · 物理学 2015-05-20 Giancarlo Ghirlanda

We probe the existence of the E_peak-E_iso correlation in long GRBs using a sample of 442 BATSE bursts with known E_peak and with redshift estimated through the lag-luminosity correlation. This sample confirms that the rest frame peak…

天体物理学 · 物理学 2009-11-10 G. Ghirlanda , G. Ghisellini , C. Firmani

Luminosity correlations of long Gamma-ray bursts (GRB) are extensively proposed as an effective complementarity to trace the Hubble diagram of Universe at high redshifts, which is of great importance to explore properties of dark energy.…

高能天体物理现象 · 物理学 2017-02-22 Guo-Jian Wang , Hai Yu , Zheng-Xiang Li , Jun-Qing Xia , Zong-Hong Zhu

We present the constraints on the cosmological parameters obtained with the $E_{\rm peak}$--$E_{\gamma}$ correlation found with the most recent sample of 19 GRBs with spectroscopically measured redshift and well determined prompt emission…

天体物理学 · 物理学 2009-11-11 G. Ghirlanda , G. Ghisellini , C. Firmani , L. Nava , F. Tavecchio , D. Lazzati

Several correlations among Gamma Ray Burst (GRB) observables with available redshifts have been recently identified. Proper evaluation and calibration of these correlations may facilitate the use of GRBs as standard candles constraining the…

天体物理学 · 物理学 2010-03-19 S. Basilakos , L. Perivolaropoulos

We use a new method of analysis to determine parameters of cosmological gamma-ray bursts (GRBs), assuming that their distribution follows the star-formation history of the universe. Spectral evolution is calculated from an external shock…

天体物理学 · 物理学 2015-06-24 M. Boettcher , C. D. Dermer

We propose how to calibrate long gamma-ray burst (GRB) correlations employing intermediate redshift data sets, instead of limiting to $z\simeq0$ catalogs. To do so, we examine the most updated observational Hubble data (OHD) and baryonic…

宇宙学与河外天体物理 · 物理学 2022-10-26 Orlando Luongo , Marco Muccino

Differently from the equivalence time between either matter and radiation or dark energy and matter, the equivalence between dark energy and radiation occurs between two subdominant fluids, since it takes place in the matter dominated…

宇宙学与河外天体物理 · 物理学 2025-07-30 Orlando Luongo , Marco Muccino

We investigate the well-measured spectral and energetic properties of 20 gamma-ray bursts (GRBs) in their cosmological rest frames. We find a tight relation between the isotropic-equivalent gamma-ray energy Eiso, the local peak energy E'p…

天体物理学 · 物理学 2007-05-23 D. Xu

The best measure of the Universe should be done using a standard "ruler" at any redshift. Type Ia Supernovae (SN Ia) probe the universe up to z$\sim$1.5, while the Cosmic Microwave Background (CMB) primary anisotropies concern basically…

天体物理学 · 物理学 2009-11-10 G. Ghirlanda , G. Ghisellini , D. Lazzati , C. Firmani

Simple hardness ratios are found to be a good estimator for the spectral peak energy in Gamma-Ray Bursts (GRBs). Specifically, a high correlation strength is found between the $\nu F_{\nu}$ peak in the spectrum of BATSE GRBs, $\epo$, and…

高能天体物理现象 · 物理学 2018-02-05 Amir Shahmoradi , Robert J. Nemiroff