STACKED SEARCH FOR GRAVITATIONAL WAVES FROM THE 2006 SGR 1900+14 STORM

被引:45
作者
Abbott, B. P. [1 ]
Abbott, R. [1 ]
Adhikari, R. [1 ]
Ajith, P. [2 ]
Allen, B. [2 ,3 ]
Allen, G. [4 ]
Amin, R. S. [5 ]
Anderson, S. B. [1 ]
Anderson, W. G. [3 ]
Arain, M. A. [6 ]
Araya, M. [1 ]
Armandula, H. [1 ]
Armor, P. [3 ]
Aso, Y. [1 ]
Aston, S. [7 ]
Aufmuth, P. [8 ]
Aulbert, C. [2 ]
Babak, S. [9 ]
Baker, P. [10 ]
Ballmer, S. [1 ]
Barker, C. [11 ]
Barker, D. [11 ]
Barr, B. [12 ]
Barriga, P. [13 ]
Barsotti, L. [14 ]
Barton, M. A. [1 ]
Bartos, I. [15 ]
Bassiri, R. [12 ]
Bastarrika, M. [12 ]
Behnke, B. [9 ]
Benacquista, M. [16 ]
Betzwieser, J. [1 ]
Beyersdorf, P. T. [17 ]
Bilenko, I. A. [18 ]
Billingsley, G. [1 ]
Biswas, R. [3 ]
Black, E. [1 ]
Blackburn, J. K. [1 ]
Blackburn, L. [14 ]
Blair, D. [13 ]
Bland, B. [11 ]
Bodiya, T. P. [14 ]
Bogue, L. [19 ]
Bork, R. [1 ]
Boschi, V. [1 ]
Bose, S. [20 ]
Brady, P. R. [3 ]
Braginsky, V. B. [18 ]
Brau, J. E. [21 ]
Bridges, D. O. [19 ]
机构
[1] CALTECH, LIGO, Pasadena, CA 91125 USA
[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[3] Univ Wisconsin, Milwaukee, WI 53201 USA
[4] Stanford Univ, Stanford, CA 94305 USA
[5] Louisiana State Univ, Baton Rouge, LA 70803 USA
[6] Univ Florida, Gainesville, FL 32611 USA
[7] Univ Birmingham, Birmingham B15 2TT, W Midlands, England
[8] Leibniz Univ Hannover, D-30167 Hannover, Germany
[9] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
[10] Montana State Univ, Bozeman, MT 59717 USA
[11] Hanford Observ, LIGO, Richland, WA 99352 USA
[12] Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland
[13] Univ Western Australia, Crawley, WA 6009, Australia
[14] MIT, LIGO, Cambridge, MA 02139 USA
[15] Columbia Univ, New York, NY 10027 USA
[16] Univ Texas Brownsville & Texas Southmost Coll, Brownsville, TX 78520 USA
[17] San Jose State Univ, San Jose, CA 95192 USA
[18] Moscow MV Lomonosov State Univ, Moscow 119992, Russia
[19] Livingston Observ, LIGO, Livingston, LA 70754 USA
[20] Washington State Univ, Pullman, WA 99164 USA
[21] Univ Oregon, Eugene, OR 97403 USA
[22] Syracuse Univ, Syracuse, NY 13244 USA
[23] Rutherford Appleton Lab, HSIC, Didcot OX11 0QX, Oxon, England
[24] Univ Maryland, College Pk, MD 20742 USA
[25] Univ Massachusetts, Amherst, MA 01003 USA
[26] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[27] Univ Michigan, Ann Arbor, MI 48109 USA
[28] Univ Sannio Benevento, I-82100 Benevento, Italy
[29] Univ Mississippi, University, MS 38677 USA
[30] Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia
[31] CALTECH, CaRT, Pasadena, CA 91125 USA
[32] Carleton Coll, Northfield, MN 55057 USA
[33] Univ Melbourne, Parkville, Vic 3010, Australia
[34] Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales
[35] Eotvos Lorand Univ, ELTE, H-1053 Budapest, Hungary
[36] Univ Salerno, I-84084 Salerno, Italy
[37] Univ Sheffield, Sheffield S10 2TN, S Yorkshire, England
[38] Penn State Univ, University Pk, PA 16802 USA
[39] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[40] So Univ & A&M Coll, Baton Rouge, LA 70813 USA
[41] Univ Rochester, Rochester, NY 14627 USA
[42] Univ Texas Austin, Austin, TX 78712 USA
[43] Australian Natl Univ, Canberra, ACT 0200, Australia
[44] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA
[45] Univ Minnesota, Minneapolis, MN 55455 USA
[46] Univ Adelaide, Adelaide, SA 5005, Australia
[47] Univ Southampton, Southampton SO17 1BJ, Hants, England
[48] Northwestern Univ, Evanston, IL 60208 USA
[49] Natl Astron Observ Japan, Tokyo 1818588, Japan
[50] Inst Appl Phys, Nizhnii Novgorod 603950, Russia
基金
美国国家科学基金会; 澳大利亚研究理事会; 美国国家航空航天局; 英国科学技术设施理事会;
关键词
gamma rays: bursts; gravitational waves; pulsars: individual (SGR 1900+14); stars: neutron; MAGNETIZED NEUTRON-STARS; SOFT GAMMA-REPEATERS;
D O I
10.1088/0004-637X/701/2/L68
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of a LIGO search for short-duration gravitational waves (GWs) associated with the 2006 March 29 SGR 1900+14 storm. A new search method is used, "stacking" the GW data around the times of individual soft-gamma bursts in the storm to enhance sensitivity for models in which multiple bursts are accompanied by GW emission. We assume that variation in the time difference between burst electromagnetic emission and potential burst GW emission is small relative to the GW signal duration, and we time-align GW excess power time-frequency tilings containing individual burst triggers to their corresponding electromagnetic emissions. We use two GW emission models in our search: a fluence-weighted model and a flat (unweighted) model for the most electromagnetically energetic bursts. We find no evidence of GWs associated with either model. Model-dependent GW strain, isotropic GW emission energy E-GW, and gamma = E-GW/E-EM upper limits are estimated using a variety of assumed waveforms. The stacking method allows us to set the most stringent model-dependent limits on transient GW strain published to date. We find E-GW upper limit estimates (at a nominal distance of 10 kpc) of between 2 x 10(45) erg and 6 x 10(50) erg depending on the waveform type. These limits are an order of magnitude lower than upper limits published previously for this storm and overlap with the range of electromagnetic energies emitted in soft gamma repeater (SGR) giant flares.
引用
收藏
页码:L68 / L74
页数:7
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