期刊信息

  • 刊名: 河北师范大学学报(自然科学版)Journal of Hebei Normal University (Natural Science)
  • 主办: 河北师范大学
  • ISSN: 1000-5854
  • CN: 13-1061/N
  • 中国科技核心期刊
  • 中国期刊方阵入选期刊
  • 中国高校优秀科技期刊
  • 华北优秀期刊
  • 河北省优秀科技期刊

Fermi/GBM伽马暴的谱能关系

  • 1. 贵州师范学院 物理与电子科学学院, 贵州 贵阳 550018;
    2. 贵州大学 明德学院, 贵州 贵阳 550025;
    3. 贵州师范大学 物理与电子科学学院, 贵州 贵阳 550001
  • DOI: 10.13763/j.cnki.jhebnu.nse.2016.06.008

On the Spectra-energy Relation in Fermi/GBM Gamma-ray Bursts

摘要/Abstract

摘要:

选取10个已知红移的单峰Fermi/GBM长暴,采用交叉相关函数计算第1与第3能道之间的相对能谱延迟(RSL).研究发现,伽马暴的RSLs分别与峰值光度和红移相关,所得结果与已报道文献中利用BATSE暴得到的结果相符合.这意味着RSL与峰值光度和红移的相关关系不受探测仪器选择效应的影响.这表明RSL可以作为一个可能的宇宙红移探测指示器用于宇宙学参数的测量.利用这些Fermi/GBM伽马暴样本,通过重新分析发现峰值能量与峰值光度、各向同性能存在较强相关.这些关系与从BATSE暴中得到的结果不一致,而与从Swift暴得到的结果符合.

Abstract:

Selecting 10 single-pulsed Fermi/GBM long gamma-ray bursts with known redshift,we use cross-correlation function (CCF) to calculate the relative spectral lag (RSL) between energy channels 1 and 3.We find that the RSLs are respectively correlated with the peak luminosity and the redshift of gamma-ray bursts,which is consistent with that of BATSE gamma-ray bursts.This shows that correlations of RSL with the peak luminosity and the redshift are not affected by the so-called selection effect of different detectors.It also suggests that the RSL can be applied as a reliable indicator to measure the basically cosmological param-eters.With the same Fermi/GBM sample,we re-analyze the correlations of peak energy with peak luminosity and isotropic energy and find that they are tightly correlated.Interestingly,these relations are inconsistent with those obtained with BATSE GRBs but consistent with those of Swift GRBs.

参考文献 38

  • [1] CUCCHIARA A.GRB 120119A Gemini-S Redshift[EB/OL].National Advisory Committee for Aeronautics:Beardmore,2012-01-19[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/12865.gcn3{GCN 12865}.
  • [2] CENKO S B.GRB 110213A Bok Telescope Redshift[EB/OL].National Advisory Committee for Aeronautics:Elia,2012-02-13[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/11708.gcn3{GCN 11708}.
  • [3] TANVIR N.GRB 100906A Gemini-N/GMOS Redshift[EB/OL].National Advisory Committee for Aeronautics:Markwardt,2010-09-06[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/11230.gcn3{GCN 11230}.
  • [4] TANVIR N.GRB 100816A Gemini-N Redshift[EB/OL].National Advisory Committee for Aeronautics:Oates,2010-06-16[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/11116.gcn3{GCN 11116}.
  • [5] CAMPANA S.GRB 100704A Redshift[EB/OL].National Advisory Committee for Aeronautics:Grupe,2010-07-04[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/10940.gcn3{GCN 10940}.
  • [6] CUVVHIARA A.GRB 10417A Gemini-N Candidate and Redshift[EB/OL].National Advisory Committee for Aeronautics:Takahashi,2010-04-17[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/10606.gcn3{GCN 10606}.
  • [7] STRATTA G,D' ELIA V,PERRI M,et al.GRB 090902B Gemini-N Redshift[EB/OL].National Advisory Committee for Aeronautics:Stratta,2009-09-02[2016-9-12].http://gcn.gsfc.nasa.gov/reports/report_249_1.pdf{GCN Report 249.1}.
  • [8] BREEVELD A.GRB 081222 Gemini-N Redshift[EB/OL].National Advisory Committee for Aeronautics:Breeveld,2008-12-22[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/8712.gcn3{GCN 8712}.
  • [9] WANG F Y,QI S,DAI Z G.The Updated Luminosity Correlations of Gamma-ray Bursts and Cosmological Implications[J].MNRAS,2011,415(4):3423-3433.doi:10.1111/j.1365-2966.2011.18961.x
  • [10] SPYROS B,LEANDROS P.Testing Gamma Ray Bursts as Standard Candles[J].MNRAS,2008,391(1):411-419.doi:10.1111/j.1365-2966.2008.13894.x
  • [11] ZHANG B,PETER M.Gamma-ray Bursts:Progress,Problems & Prospects[J].IJMPA,2004,19(15):2385Z.doi:10.1142/SO217751X0401746X
  • [12] LI Z,DAI Z G,LU T.Gamma射线暴研究概况[J].天文学进展,2003,21(4):334-368.doi:10.8349/j.issn.1000.2003.04.05
  • [13] NORRIS J P,NEMIROFF R J,BONNELL J T,et al.Attributes of Pulses in Long Bright Gamma-ray Bursts[J].ApJ,1996,459(3):393-400.doi:10.1086/176902
  • [14] RIESS A G,FILIPPENKO A V,CHALLIS P,et al.Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant[J].ApJ,1998,116(3):1009-1038.doi:10.1086/300499
  • [15] PERLMUTTER S,ALDERING G,GOLDHABER G,et al.Measurements of Omega and Lambda from 42 High-redshift Supernovae[J].ApJ,1999,517(2):565-586.doi:10.1086/307221
  • [16] TEGMARK M,EISENSTEIN D J,STRAUSS M A,et al.Cosmological Constraints from the SDSS Luminous Red Galaxies[J].Phys Rev,2006,74(12):123507.doi:10.1103/PhysRevD.74.123507
  • [17] DAVIS T M,MÖRTSELL E,SOLLERMAN J,et al.Scrutinizing Exotic Cosmological Models Using Essence Supernova Data Combined with Other Cosmological Probes[J].ApJ,2007,666(2):716-725.doi:10.1086/519988
  • [18] GHIRLANDA G,GHISELLINI G,LAZZATI D.The Collimation-corrected Gamma-ray Burst Energies Correlate with the Peak Energy of Their γFγ Spectrum[J].ApJ,2004,616(1):331-338.doi:10.1086/424913
  • [19] AMATI L,FRONTERA F,TAVANI M,et al.Intrinsic Spectra and Energetics of Beppo SAX Gamma-ray Bursts with Known Redshifts[J].A&A,2002,390:81-89.doi:10.1051/0004-6361:200220722
  • [20] NORRIS J P,MARANI G F,BONNELL J.Connection Between Energy-dependent Lags and Peak Luminosity in Gamma-ray Bursts[J].ApJ,2000,534(1):248-257.doi:10.1086/308725
  • [21] FENIMORE E E.The Average Temporal and Spectral Evolution of Gamma-ray Bursts[J].ApJ,1999,518(1):375-379.doi:10.1086/307245
  • [22] SCHAEFER B E.Gamma-ray Burst Hubble Diagram to z=4.5[J].ApJ,2003,583(2):L67-L70.doi:10.1086/368104
  • [23] PENG Z Y,LU R J,QIN Y P,et al.Relationships Between Relative Spectral Lags and Relative Widths of Gamma-ray Bursts[J].CHJAA,2007,7(3):428-434.doi:10.1088/1009-9271/7/3/13
  • [24] NORRIS J P,MARANI G F,BONNELL J.Connection Between Energy-dependent Lags and Peak Luminosity in Gamma-ray Bursts[J].ApJ,2000,534(1):248-434.doi:10.1086/308725
  • [25] UKWATTA T N,STAMATIKOS M,DHUGA K S,et al.Spectral Lags and the Lag-luminosity Relation:An Investigation with Swift BAT Gamma-ray Bursts[J].ApJ,2010,711(2):1073-1086.doi:10.1088/0004-637X/711/2/1073
  • [26] ZHANG Z B,DENG J G,LU R J,et al.Relative Spectral Lag:A New Redshift Indicator of Gamma-ray Bursts[J].CHJAA,2006,6(3):312-322.doi:10.1088/1009-9271/6/3/06
  • [27] ZHANG Z B,XIE G Z,CHOI C S.Testing a New Luminosity/redshift Estimator of GRBs[J].IJMPD,2008,17(9):1391-1399.doi:10.1142/SO218271808012966
  • [28] 张义贞,张志彬.Swift伽玛暴的谱延迟距离指示器[J].贵州大学学报,2012,29(1):30-34.doi:10.15958/j.cnki.gdxbzrb.2012.01.030
  • [29] AMATI L.The Ep,i-Eiso Correlation in Gamma-ray Bursts:Updated Observational Status,Re-analysis and Main Implications[J].MNRAS,2006,372(1):233245.doi:10.1111/j.1365-2966.2006.10840.x
  • [30] WEI D M,GAO W H.Are There Cosmological Evolution Trends on Gamma-ray Burst Features[J].MNRAS, 2003,345(3):743-746.doi:10.1046/j.1365-8711.2003.06971.x
  • [31] YONETOKU D,MURAKAMI T,NAKAMURA T,et al.Gamma-ray Burst Formation Rate Inferred from the Spectral Peak Energy-peak Luminosity Relation[J].ApJ,2004,609(2):935-951.doi:10.1086/421285
  • [32] ZHANG Z B,CHEN D Y,HUANG Y F.Correlation Between Peak Energy and Peak Luminosity in Short Gamma-ray Bursts[J].ApJ,2012,755(1):1-7.doi:10.1088/0004-637X/755/1/5
  • [33] KOCEVSKI D,RYDE F,LIANG E.Search for Relativistic Curvature Effects in Gamma-ray Burst Pulses[J].ApJ,2003,596(1):389-400.doi:10.1086/377707
  • [34] BAND D L.Gamma-ray Burst Spectral Evolution Through Cross-correlations of Discriminator Light Curves[J].ApJ,1997,486(2):928-937.doi:10.1086/198623
  • [35] GRUBER D,ADAM G,VICTORIA W von A,et al.The Fermi GBM Gamma-ray Burst Catalog:The First Four Years[J].ApJ,2014,211(1):12-13.doi:10.1088/0067-0049/211/1/12
  • [36] KIENLIN von A.MEEGAN W S P.The Second Fermi GBM Gamma-ray Burst Catalog:The First Four Years[J].ApJ,2014,211(1):13-14.doi:10.1088/0067-0049/211/1/13
  • [37] TANVIR N R,BALL J.GRB 120729A Gemini-N Redshift[EB/OL].National Advisory Committee for Aeronautics:Ukwatta,2012-07-29[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/13532.gcn3{GCN 13532}.
  • [38] CASTRO-TIRADO A.GRB 120326A GTC Redshift[EB/OL].National Advisory Committee for Aeronautics:Siegel,2012-03-26[2016-9-12].http://gcn.gsfc.nasa.gov/gcn3/13118.gcn3{GCN 13118}.