Beating the spin-down limit on gravitational wave emission from the crab pulsar


Abbott, B., Abbott, R., Adhikari, R., Ajith, P., Allen, B., Allen, G., Amin, R., Anderson, S.B., Anderson, W.G., Arain, M.A., Araya, M., Armandula, H., Armor, P., Aso, Y., Aston, S., Aufmuth, P., Aulbert, C., Babak, S., Ballmer, S., Bantilan, H., Barish, B.C., Barker, C., Barker, D., Barr, B., Barriga, P., Barton, M.A., Bastarrika, M., Bayer, K., Betzwieser, J., Beyersdorf, P.T., Bilenko, I.A., Billingsley, G., Biswas, R., Black, E., Blackburn, K., Blackburn, L., Blair, D., Bland, B., Bodiya, T.P., Bogue, L., Bork, R., Boschi, V., Bose, S., Brady, P.R., Braginsky, V.B., Brau, J.E., Brinkmann, M., Brooks, A., Brown, D.A., Brunet, G., Bullington, A., Buonanno, A., Burmeister, O., Byer, R.L., Cadonati, L., Cagnoli, G., Camp, J.B., Cannizzo, J., Cannon, K., Cao, J., Cardenas, L., Casebolt, T., Castaldi, G., Cepeda, C., Chalkley, E., Charlton, P., Chatterji, S., Chelkowski, S., Chen, Y., Christensen, N., Clark, D., Clark, J., Cokelaer, T., Conte, R., Cook, D., Corbitt, T., Coyne, D., Creighton, J.D.E., Cumming, A., Cunningham, L., Cutler, R.M., Dalrymple, J., Danzmann, K., Davies, G., DeBra, D., Degallaix, J., Degree, M., Dergachev, V., Desai, S., DeSalvo, R., Dhurandhar, S., Díaz, M., Dickson, J., Dietz, A., Donovan, F., Dooley, K.L., Doomes, E.E., Drever, R.W.P., Duke, I., Dumas, J.-C., Dupuis, R.J., Dwyer, J.G., Echols, C., Effler, A., Ehrens, P., Espinoza, E., Etzel, T., Evans, T., Fairhurst, S., Fan, Y., Fazi, D., Fehrmann, H., Fejer, M.M., Finn, L.S., Flasch, K., Fotopoulos, N., Freise, A., Frey, R., Fricke, T., Fritschel, P., Frolov, V.V., Fyffe, M., Garofoli, J., Gholami, I., Giaime, J.A., Giampanis, S., Giardina, K.D., Goda, K., Goetz, E., Goggin, L., González, G., Gossler, S., Gouaty, R., Grant, A., Gras, S., Gray, C., Gray, M., Greenhalgh, R.J.S., Gretarsson, A.M., Grimaldi, F., Grosso, R., Grote, H., Grunewald, S., Guenther, M., Gustafson, E.K., Gustafson, R., Hage, B., Hallam, J.M., Hammer, D., Hanna, C., Hanson, J., Harms, J., Harry, G., Harstad, E., Hayama, K., Hayler, T., Heefner, J., Heng, I.S., Hennessy, M., Heptonstall, A., Hewitson, M., Hild, S., Hirose, E., Hoak, D., Hosken, D., Hough, J., Huttner, S.H., Ingram, D., Ito, M., Ivanov, A., Johnson, B., Johnson, W.W., Jones, D.I., Jones, G., Jones, R., Ju, L., Kalmus, P., Kalogera, V., Kamat, S., Kanner, J., Kasprzyk, D., Katsavounidis, E., Kawabe, K., Kawamura, S., Kawazoe, F., Kells, W., Keppel, D.G., Khalili, F.Ya., Khan, R., Khazanov, E., Kim, C., King, P., Kissel, J.S., Klimenko, S., Kokeyama, K., Kondrashov, V., Kopparapu, R.K., Kozak, D., Kozhevatov, I., Krishnan, B., Kwee, P., Lam, P.K., Landry, M., Lang, M.M., Lantz, B., Lazzarini, A., Lei, M., Leindecker, N., Leonhardt, V., Leonor, I., Libbrecht, K., Lin, H., Lindquist, P., Lockerbie, N.A., Lodhia, D., Lormand, M., Lu, P., Lubinski, M., Lucianetti, A., Lück, H., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Mandic, V., Márka, S., Márka, Z., Markosyan, A., Markowitz, J., Maros, E., Martin, I., Martin, R.M., Marx, J.N., Mason, K., Matichard, F., Matone, L., Matzner, R., Mavalvala, N., McCarthy, R., McClelland, D.E., McGuire, S.C., McHugh, M., McIntyre, G., McIvor, G., McKechan, D., McKenzie, K., Meier, T., Melissinos, A., Mendell, G., Mercer, R.A., Meshkov, S., Messenger, C.J., Meyers, D., Miller, J., Minelli, J., Mitra, S., Mitrofanov, V.P., Mitselmakher, G., Mittleman, R., Miyakawa, O., Moe, B., Mohanty, S., Moreno, G., Mossavi, K., MowLowry, C., Mueller, G., Mukherjee, S., Mukhopadhyay, H., Müller-Ebhardt, H., Munch, J., Murray, P., Myers, E., Myers, J., Nash, T., Nelson, J., Newton, G., Nishizawa, A., Numata, K., O'Dell, J., Ogin, G., O'Reilly, B., O'Shaughnessy, R., Ottaway, D.J., Ottens, R.S., Overmier, H., Owen, B.J., Pan, Y., Pankow, C., Papa, M.A., Parameshwaraiah, V., Patel, P., Pedraza, M., Penn, S., Perreca, A., Petrie, T., Pinto, I.M., Pitkin, M., Pletsch, H.J., Plissi, M.V., Postiglione, F., Principe, M., Prix, R., Quetschke, V., Raab, F., Rabeling, D.S., Radkins, H., Rainer, N., Rakhmanov, M., Ramsunder, M., Rehbein, H., Reid, S., Reitze, D.H., Riesen, R., Riles, K., Rivera, B., Robertson, N.A., Robinson, C., Robinson, E.L., Roddy, S., Rodriguez, A., Rogan, A.M., Rollins, J., Romano, J.D., Romie, J., Route, R., Rowan, S., Rüdiger, A., Ruet, L., Russell, P., Ryan, K., Sakata, S., Samidi, M., de la Jordana, L. Sancho, Sandberg, V., Sannibale, V., Saraf, S., Sarin, P., Sathyaprakash, B.S., Sato, S., Saulson, P.R., Savage, R., Savov, P., Schediwy, S.W., Schilling, R., Schnabel, R., Schofield, R., Schutz, B.F., Schwinberg, P., Scott, S.M., Searle, A.C., Sears, B., Seifert, F., Sellers, D., Sengupta, A.S., Shawhan, P., Shoemaker, D.H., Sibley, A., Siemens, X., Sigg, D., Sinha, S., Sintes, A.M., Slagmolen, B.J.J., Slutsky, J., Smith, J.R., Smith, M.R., Smith, N.D., Somiya, K., Sorazu, B., Stein, L.C., Stochino, A., Stone, R., Strain, K.A., Strom, D.M., Stuver, A., Summerscales, T.Z., Sun, K.-X., Sung, M., Sutton, P.J., Takahashi, H., Tanner, D.B., Taylor, R., Thacker, J., Thorne, K.A., Thorne, K.S., Thüring, A., Tokmakov, K.V., Torres, C., Torrie, C., Traylor, G., Trias, M., Tyler, W., Ugolini, D., Ulmen, J., Urbanek, K., Vahlbruch, H., Van Den Broeck, C., van der Sluys, M., Vass, S., Vaulin, R., Vecchio, A., Veitch, J., Veitch, P., Villar, A., Vorvick, C., Vyachanin, S.P., Waldman, S.J., Wallace, L., Ward, H., Ward, R., Weinert, M., Weinstein, A., Weiss, R., Wen, S., Wette, K., Whelan, J.T., Whitcomb, S.E., Whiting, B.F., Wilkinson, C., Willems, P.A., Williams, H.R., Williams, L., Willke, B., Wilmut, I., Winkler, W., Wipf, C.C., Wiseman, A.G., Woan, G., Wooley, R., Worden, J., Wu, W., Yakushin, I., Yamamoto, H., Yan, Z., Yoshida, S., Zanolin, M., Zhang, J., Zhang, L., Zhao, C., Zotov, N., Zucker, M., Zweizig, J. and Santostasi, G. (2008) Beating the spin-down limit on gravitational wave emission from the crab pulsar The Astrophysical Journal Letters, 683, (1), L45-L49. (doi:10.1086/591526).

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Description/Abstract

We present direct upper limits on gravitational wave emission from the Crab pulsar using data from the first 9 months of the fifth science run of the Laser Interferometer Gravitational-wave Observatory (LIGO). These limits are based on two searches. In the first we assume that the gravitational wave emission follows the observed radio timing, giving an upper limit on gravitational wave emission that beats indirect limits inferred from the spin-down and braking index of the pulsar and the energetics of the nebula. In the second we allow for a small mismatch between the gravitational and radio signal frequencies and interpret our results in the context of two possible gravitational wave emission mechanisms.

Item Type: Article
Digital Object Identifier (DOI): doi:10.1086/591526
Subjects: Q Science > QA Mathematics
ePrint ID: 154877
Date :
Date Event
18 July 2008e-pub ahead of print
10 August 2008Published
Date Deposited: 26 May 2010 14:44
Last Modified: 18 Apr 2017 04:06
Further Information:Google Scholar
URI: http://eprints.soton.ac.uk/id/eprint/154877

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