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Search for gravitational waves from primordial black hole binary coalescences in the galactic halo

Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Allen, B., Amin, R., Anderson, S., Anderson, W., Araya, M., Armandula, H., Ashley, M., Asiri, F., Aufmuth, P., Aulbert, C., Babak, Stanislav, Balasubramanian, Ramachandran, Ballmer, S., Barish, B., Barker, C., Barker, D., Barnes, M., Barr, B., Barton, M., Bayer, K., Beausoleil, R., Belczynski, K., Bennett, R., Berukoff, S., Betzwieser, J., Bhawal, B., Bilenko, I., Billingsley, G., Black, E., Blackburn, K., Blackburn, L., Bland, B., Bochner, B., Bogue, L., Bork, R., Bose, S., Brady, P., Braginsky, V., Brau, J., Brown, D., Bullington, A., Bunkowski, A., Buonanno, A., Burgess, R., Busby, D., Butler, W., Byer, R., Cadonati, L., Cagnoli, G., Camp, J., Cantley, C., Cardenas, L., Carter, K., Casey, M., Castiglione, J., Chandler, A., Chapsky, J., Charlton, P., Chatterji, S., Chelkowski, S., Chen, Y., Chickarmane, V., Chin, D., Christensen, N., Churches, David K., Cokelaer, Thomas, Colacino, C., Coldwell, R., Coles, M., Cook, D., Corbitt, T., Coyne, D., Creighton, J., Creighton, T., Crooks, D., Csatorday, P., Cusack, B., Cutler, C., D'Ambrosio, E., Danzmann, K., Daw, E., DeBra, D., Delker, T., Dergachev, V., DeSalvo, R., Dhurandhar, S., Credico, A., Díaz, M., Ding, H., Drever, R., Dupuis, R., Edlund, J., Ehrens, P., Elliffe, E., Etzel, T., Evans, M., Evans, T., Fairhurst, Stephen ORCID: https://orcid.org/0000-0001-8480-1961, Fallnich, C., Farnham, D., Fejer, M., Findley, T., Fine, M., Finn, L., Franzen, K., Freise, A., Frey, R., Fritschel, P., Frolov, V., Fyffe, M., Ganezer, K., Garofoli, J., Giaime, J., Gillespie, A., Goda, K., González, G., Goßler, S., Grandclément, P., Grant, A., Gray, C., Gretarsson, A., Grimmett, D., Grote, H., Grunewald, S., Guenther, M., Gustafson, E., Gustafson, R., Hamilton, W., Hammond, M., Hanson, J., Hardham, C., Harms, J., Harry, G., Hartunian, A., Heefner, J., Hefetz, Y., Heinzel, G., Heng, I., Hennessy, M., Hepler, N., Heptonstall, A., Heurs, M., Hewitson, M., Hild, S., Hindman, N., Hoang, P., Hough, J., Hrynevych, M., Hua, W., Ito, M., Itoh, Y., Ivanov, A., Jennrich, O., Johnson, B., Johnson, W., Johnston, W., Jones, D., Jones, L., Jungwirth, D., Kalogera, V., Katsavounidis, E., Kawabe, K., Kawamura, S., Kells, W., Kern, J., Khan, A., Killbourn, S., Killow, C., Kim, C., King, C., King, P., Klimenko, S., Koranda, S., Kötter, K., Kovalik, J., Kozak, D., Krishnan, B., Landry, M., Langdale, J., Lantz, B., Lawrence, R., Lazzarini, A., Lei, M., Leonor, I., Libbrecht, K., Libson, A., Lindquist, P., Liu, S., Logan, J., Lormand, M., Lubinski, M., Lück, H., Lyons, T., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Majid, W., Malec, M., Mann, F., Marin, A., Márka, S., Maros, E., Mason, J., Mason, K., Matherny, O., Matone, L., Mavalvala, N., McCarthy, R., McClelland, D., McHugh, M., McNabb, J., Mendell, G., Mercer, R., Meshkov, S., Messaritaki, Eirini ORCID: https://orcid.org/0000-0002-9917-4160, Messenger, Christopher, Mitrofanov, V., Mitselmakher, G., Mittleman, R., Miyakawa, O., Miyoki, S., Mohanty, S., Moreno, G., Mossavi, K., Mueller, G., Mukherjee, S., Murray, P., Myers, J., Nagano, S., Nash, T., Nayak, R., Newton, G., Nocera, F., Noel, J., Nutzman, P., Olson, T., O'Reilly, B., Ottaway, D., Ottewill, A., Ouimette, D., Overmier, H., Owen, B., Pan, Y., Papa, M., Parameshwaraiah, V., Parameswaran, A., Parameswariah, C., Pedraza, M., Penn, S., Pitkin, M., Plissi, M., Prix, R., Quetschke, V., Raab, F., Radkins, H., Rahkola, R., Rakhmanov, M., Rao, S., Rawlins, K., Ray-Majumder, S., Re, V., Redding, D., Regehr, M., Regimbau, Tania, Reid, S., Reilly, K., Reithmaier, K., Reitze, D., Richman, S., Riesen, R., Riles, K., Rivera, B., Rizzi, A., Robertson, D., Robertson, N., Robison, L., Roddy, S., Rollins, J., Romano, Joseph David, Romie, J., Rong, H., Rose, D., Rotthoff, E., Rowan, S., Rüdiger, A., Russell, P., Ryan, K., Salzman, I., Sandberg, V., Sanders, G., Sannibale, V., Sathyaprakash, Bangalore Suryanarayana ORCID: https://orcid.org/0000-0003-3845-7586, Saulson, P., Savage, R., Sazonov, A., Schilling, R., Schlaufman, K., Schmidt, V., Schnabel, R., Schofield, R., Schutz, Bernard ORCID: https://orcid.org/0000-0001-9487-6983, Schwinberg, P., Scott, S., Seader, S., Searle, A., Sears, B., Seel, S., Seifert, F., Sengupta, A., Shapiro, C., Shawhan, P., Shoemaker, D., Shu, Q., Sibley, A., Siemens, X., Sievers, L., Sigg, D., Sintes, A., Smith, J., Smith, M., Smith, M., Sneddon, P., Spero, R., Stapfer, G., Steussy, D., Strain, K., Strom, D., Stuver, A., Summerscales, T., Sumner, M., Sutton, P., Sylvestre, J., Takamori, A., Tanner, D., Tariq, H., Taylor, I., Taylor, R., Taylor, R., Thorne, K., Thorne, K., Tibbits, M., Tilav, S., Tinto, M., Tokmakov, K., Torres, C., Torrie, C., Traylor, G., Tyler, W., Ugolini, D., Ungarelli, C., Vallisneri, M., van Putten, M., Vass, S., Vecchio, A., Veitch, J., Vorvick, C., Vyachanin, S., Wallace, L., Walther, H., Ward, H., Ware, B., Watts, K., Webber, D., Weidner, A., Weiland, U., Weinstein, A., Weiss, R., Welling, H., Wen, L., Wen, S., Whelan, J., Whitcomb, S., Whiting, B., Wiley, S., Wilkinson, C., Willems, P., Williams, P., Williams, R., Willke, B., Wilson, A., Winjum, B., Winkler, W., Wise, S., Wiseman, A., Woan, G., Woods, D., Wooley, R., Worden, J., Wu, W., Yakushin, I., Yamamoto, H., Yoshida, S., Zaleski, K., Zanolin, M., Zawischa, I., Zhang, L., Zhu, R., Zotov, N., Zucker, M. and Zweizig, J. 2005. Search for gravitational waves from primordial black hole binary coalescences in the galactic halo. Physical Review D 72 (8) , 082002. 10.1103/PhysRevD.72.082002

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Abstract

We use data from the second science run of the LIGO gravitational-wave detectors to search for the gravitational waves from primordial black hole binary coalescence with component masses in the range 0.2–1.0M⊙. The analysis requires a signal to be found in the data from both LIGO observatories, according to a set of coincidence criteria. No inspiral signals were found. Assuming a spherical halo with core radius 5 kpc extending to 50 kpc containing nonspinning black holes with masses in the range 0.2–1.0M⊙, we place an observational upper limit on the rate of primordial black hole coalescence of 63 per year per Milky Way halo (MWH) with 90% confidence.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Cardiff University Brain Research Imaging Centre (CUBRIC)
Medicine
Physics and Astronomy
Psychology
Subjects: Q Science > QB Astronomy
Publisher: American Physical Society
ISSN: 1550-7998
Last Modified: 21 Oct 2022 09:22
URI: https://orca.cardiff.ac.uk/id/eprint/36099

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