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1. Astrophysics with the Laser Interferometer Space Antenna

Author

Seoane, Pau Amaro, Andrews, Jeff, Sedda, Manuel Arca, Askar, Abbas, Baghi, Quentin, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stephane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katelyn, Capelo, Pedro R., Caramete, Laurentiu, Cattorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ross, Colpi, Monica, D'Orazio, Daniel, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriakos, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Franchini, Alessia, Fragos, Tassos, Fryer, Chris, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul, Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Tomas, Kokkotas, Kostas, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thomas, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Tomas, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Steéphane, Mayer, Lucio, McGee, Sean, McKernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S, Nelemans, Gijs, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileio, Pfister, Hugo, Porquet, Delphine, Quenby, John, Ricarte, Angelo, Röpke, Friedrich K., Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Raffaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlos, Stone, Nicholas C., Suvorov, Arthur, Tamanini, Nicola, Tamfal, Tomas, Tauris, Thomas, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonios, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Rivera, Alexander Bonilla, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Fragione, Giacomo, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O'Shaughnessy, Richard, Zwart, Simon Portegies, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, and Vigna-Gómez, Alejandro

Subjects
General Relativity and Quantum Cosmology, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA's first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultracompact stellar-mass binaries, massive black hole binaries, and extreme or intermediate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe.

Published
2022
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2. Astrophysics with the Laser Interferometer Space Antenna

Author

Amaro-Seoane, Pau, Andrews, Jeff, Arca Sedda, Manuel, Askar, Abbas, Baghi, Quentin, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stéphane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katelyn, Capelo, Pedro R., Caramete, Laurentiu, Cattorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ross, Colpi, Monica, D’Orazio, Daniel, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriakos, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Franchini, Alessia, Fragos, Tassos, Fryer, Chris, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul, Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Tomas, Kokkotas, Kostas, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thomas, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Tomas, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Stéphane, Mayer, Lucio, McGee, Sean, McKernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S., Nelemans, Gijs, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileios, Pfister, Hugo, Porquet, Delphine, Quenby, John, Ricarte, Angelo, Röpke, Friedrich K., Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Raffaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlos, Stone, Nicholas C., Suvorov, Arthur, Tamanini, Nicola, Tamfal, Tomas, Tauris, Thomas, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonios, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Bonilla Rivera, Alexander, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O’Shaughnessy, Richard, Portegies Zwart, Simon, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, and Vigna-Gómez, Alejandro

Published
2023
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3. The Cherenkov Telescope Array On-Site integral sensitivity: observing the Crab

Author

Fioretti, Valentina, Bulgarelli, Andrea, and Schussler, Fabian

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

The Cherenkov Telescope Array (CTA) is the future large observatory in the very high energy (VHE) domain. Operating from 20 GeV to 300 TeV, it will be composed of tens of Imaging Air Cherenkov Telescopes (IACTs) displaced in a large area of a few square kilometers in both the southern and northern hemispheres. The CTA/DATA On-Site Analysis (OSA) is the system devoted to the development of dedicated pipelines and algorithms to be used at the CTA site for the reconstruction, data quality monitoring, science monitoring and realtime science alerting during observations. The OSA integral sensitivity is computed here for the most studied source at Gamma-rays, the Crab Nebula, for a set of exposures ranging from 1000 seconds to 50 hours, using the full CTA Southern array. The reason for the Crab Nebula selection as the first example of OSA integral sensitivity is twofold: (i) this source is characterized by a broad spectrum covering the entire CTA energy range; (ii) it represents, at the time of writing, the standard candle in VHE and it is often used as unit for the IACTs sensitivity. The effect of different Crab Nebula emission models on the CTA integral sensitivity is evaluated, to emphasize the need for representative spectra of the CTA science targets in the evaluation of the OSA use cases. Using the most complete model as input to the OSA integral sensitivity, we obtain a significant detection of the Crab nebula (about 10% of flux) even for a 1000 second exposure, for an energy threshold less than 10 TeV.

Published
2016
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4. Astrophysics with the Laser Interferometer Space Antenna

Author

Seoane, Pau Amaro, Andrews, Jeff, Sedda, Manuel Arca, Askar, Abbas, Baghi, Quentin, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stephane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katelyn, Capelo, Pedro R., Caramete, Laurentiu, Cattorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ross, Colpi, Monica, D'Orazio, Daniel, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriakos, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Franchini, Alessia, Fragos, Tassos, Fryer, Chris, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul, Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Tomas, Kokkotas, Kostas, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thomas, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Tomas, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Steéphane, Mayer, Lucio, McGee, Sean, McKernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S, Nelemans, Gijs, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileio, Pfister, Hugo, Porquet, Delphine, Quenby, John, Ricarte, Angelo, Röpke, Friedrich K., Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Raffaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlos, Stone, Nicholas C., Suvorov, Arthur, Tamanini, Nicola, Tamfal, Tomas, Tauris, Thomas, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonios, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Rivera, Alexander Bonilla, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Fragione, Giacomo, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O'Shaughnessy, Richard, Zwart, Simon Portegies, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, Vigna-Gómez, Alejandro, Amaro-Seoane, Pau, Andrews, Jeff, Arca Sedda, Manuel, Askar, Abba, Baghi, Quentin, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stéphane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katelyn, Capelo, Pedro R., Caramete, Laurentiu, Cattorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ro, Colpi, Monica, D’Orazio, Daniel, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriako, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Franchini, Alessia, Fragos, Tasso, Fryer, Chri, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul, Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Toma, Kokkotas, Kosta, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thoma, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Toma, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Stéphane, Mayer, Lucio, Mcgee, Sean, Mckernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S., Nelemans, Gij, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileio, Pfister, Hugo, Porquet, Delphine, Quenby, John, Ricarte, Angelo, Röpke, Friedrich K., Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Raffaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlo, Stone, Nicholas C., Suvorov, Arthur, Tamanini, Nicola, Tamfal, Toma, Tauris, Thoma, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonio, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Bonilla Rivera, Alexander, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O’Shaughnessy, Richard, Portegies Zwart, Simon, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, Vigna-Gómez, Alejandro, Max Planck Institute for Gravitational Physics (Albert Einstein Institute) (AEI), Max-Planck-Gesellschaft, Institut de Ciencies de l'Espai [Barcelona] (ICE-CSIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Department of Physics, Columbia University, Columbia University [New York], Department of Physics and Astronomy [Nashville], Vanderbilt University [Nashville], Fisk University, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire des deux Infinis de Toulouse (L2IT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Amaro-Seoane, P, Andrews, J, Arca Sedda, M, Askar, A, Baghi, Q, Balasov, R, Bartos, I, Bavera, S, Bellovary, J, Berry, C, Berti, E, Bianchi, S, Blecha, L, Blondin, S, Bogdanović, T, Boissier, S, Bonetti, M, Bonoli, S, Bortolas, E, Breivik, K, Capelo, P, Caramete, L, Cattorini, F, Charisi, M, Chaty, S, Chen, X, Chruślińska, M, Chua, A, Church, R, Colpi, M, D’Orazio, D, Danielski, C, Davies, M, Dayal, P, De Rosa, A, Derdzinski, A, Destounis, K, Dotti, M, Duţan, I, Dvorkin, I, Fabj, G, Foglizzo, T, Ford, S, Fouvry, J, Franchini, A, Fragos, T, Fryer, C, Gaspari, M, Gerosa, D, Graziani, L, Groot, P, Habouzit, M, Haggard, D, Haiman, Z, Han, W, Istrate, A, Johansson, P, Khan, F, Kimpson, T, Kokkotas, K, Kong, A, Korol, V, Kremer, K, Kupfer, T, Lamberts, A, Larson, S, Lau, M, Liu, D, Lloyd-Ronning, N, Lodato, G, Lupi, A, Ma, C, Maccarone, T, Mandel, I, Mangiagli, A, Mapelli, M, Mathis, S, Mayer, L, Mcgee, S, Mckernan, B, Miller, M, Mota, D, Mumpower, M, Nasim, S, Nelemans, G, Noble, S, Pacucci, F, Panessa, F, Paschalidis, V, Pfister, H, Porquet, D, Quenby, J, Ricarte, A, Röpke, F, Regan, J, Rosswog, S, Ruiter, A, Ruiz, M, Runnoe, J, Schneider, R, Ministerio de Ciencia e Innovación (España), European Research Council, European Commission, Istituto Nazionale di Astrofisica, Agenzia Spaziale Italiana, and National Aeronautics and Space Administration (US)

Subjects
Astrofísica, ACTIVE GALACTIC NUCLEI, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics and Astronomy (miscellaneous), Black hole, Astronomy, Stellar remnant, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), TIDAL DISRUPTION EVENTS, General Relativity and Quantum Cosmology, Gravitational waves, MOCCA-SURVEY DATABASE, Settore FIS/05 - Astronomia e Astrofisica, Stellar remnants, Software Science, Multi-messenger, GRAVITATIONAL-WAVE SOURCES, Instrumentation and Methods for Astrophysics (astro-ph.IM), Extreme mass ratio in-spirals, Solar and Stellar Astrophysics (astro-ph.SR), High Energy Astrophysical Phenomena (astro-ph.HE), Black holes, Data Science, Astrophysics::Instrumentation and Methods for Astrophysics, Extreme mass ratio in-spiral, AM-CVN STARS, Astrophysics - Astrophysics of Galaxies, WHITE-DWARF BINARIES, DOUBLE NEUTRON-STARS, Astrophysics - Solar and Stellar Astrophysics, [SDU]Sciences of the Universe [physics], Astrophysics of Galaxies (astro-ph.GA), Astronomia, MASSIVE BLACK-HOLE, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, X-RAY BINARIES, COMMON-ENVELOPE EVOLUTION, Gravitational wave, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Full list of authors: Amaro-Seoane, Pau; Andrews, Jeff; Sedda, Manuel Arca; Askar, Abbas.; Baghi, Quentin; Balasov, Razvan; Bartos, Imre; Bavera, Simone S.; Bellovary, Jillian; Berry, Christopher P. L.; Berti, Emanuele; Bianchi, Stefano; Blecha, Laura; Blondin, Stephane; Bogdanovic, Tamara; Boissier, Samuel; Bonetti, Matteo; Bonoli, Silvia; Bortolas, Elisa; Breivik, Katelyn; Capelo, Pedro R.; Caramete, Laurentiu; Cattorini, Federico; Charisi, Maria; Chaty, Sylvain; Chen, Xian; Chruslinska, Martyna; Chua, Alvin J. K.; Church, Ross; Colpi, Monica; D'Orazio, Daniel; Danielski, Camilla; Davies, Melvyn B.; Dayal, Pratika; De Rosa, Alessandra; Derdzinski, Andrea; Destounis, Kyriakos; Dotti, Massimo; Dutan, Ioana; Dvorkin, Irina; Fabj, Gaia; Foglizzo, Thierry; Ford, Saavik; Fouvry, Jean-Baptiste; Franchini, Alessia; Fragos, Tassos; Fryer, Chris; Gaspari, Massimo; Gerosa, Davide; Graziani, Luca; Groot, Paul; Habouzit, Melanie; Haggard, Daryl; Haiman, Zoltan; Han, Wen-Biao; Istrate, Alina; Johansson, Peter H.; Khan, Fazeel Mahmood; Kimpson, Tomas; Kokkotas, Kostas; Kong, Albert; Korol, Valeriya; Kremer, Kyle; Kupfer, Thomas; Lamberts, Astrid; Larson, Shane; Lau, Mike; Liu, Dongliang; Lloyd-Ronning, Nicole; Lodato, Giuseppe; Lupi, Alessandro; Ma, Chung-Pei; Maccarone, Tomas; Mandel, Ilya; Mangiagli, Alberto; Mapelli, Michela; Mathis, Stephane; Mayer, Lucio; McGee, Sean; McKernan, Berry; Miller, M. Coleman; Mota, David F.; Mumpower, Matthew; Nasim, Syeda S.; Nelemans, Gijs; Noble, Scott; Pacucci, Fabio; Panessa, Francesca; Paschalidis, Vasileios; Pfister, Hugo; Porquet, Delphine; Quenby, John; Ricarte, Angelo; Roepke, Friedrich K.; Regan, John; Rosswog, Stephan; Ruiter, Ashley; Ruiz, Milton; Runnoe, Jessie; Schneider, Raffaella; Schnittman, Jeremy; Secunda, Amy; Sesana, Alberto; Seto, Naoki; Shao, Lijing; Shapiro, Stuart; Sopuerta, Carlos; Stone, Nicholas C.; Suvorov, Arthur; Tamanini, Nicola; Tamfal, Tomas; Tauris, Thomas; Temmink, Karel; Tomsick, John; Toonen, Silvia; Torres-Orjuela, Alejandro; Toscani, Martina; Tsokaros, Antonios; Unal, Caner; Vazquez-Aceves, Veronica; Valiante, Rosa; van Putten, Maurice; van Roestel, Jan; Vignali, Christian; Volonteri, Marta; Wu, Kinwah; Younsi, Ziri; Yu, Shenghua; Zane, Silvia; Zwick, Lorenz; Antonini, Fabio; Baibhav, Vishal; Barausse, Enrico; Bonilla Rivera, Alexander; Branchesi, Marica; Branduardi-Raymont, Graziella; Burdge, Kevin; Chakraborty, Srija; Cuadra, Jorge; Dage, Kristen; Davis, Benjamin; de Mink, Selma E.; Decarli, Roberto; Doneva, Daniela; Escoffier, Stephanie; Gandhi, Poshak; Haardt, Francesco; Lousto, Carlos O.; Nissanke, Samaya; Nordhaus, Jason; O'Shaughnessy, Richard; Portegies Zwart, Simon; Pound, Adam; Schussler, Fabian; Sergijenko, Olga; Spallicci, Alessandro; Vernieri, Daniele; Vigna-Gomez, Alejandro.-- This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/., The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA’s first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultra-compact stellar-mass binaries, massive black hole binaries, and extreme or interme-diate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe. © The Author(s) 2023, corrected publication 2023., P. Dayal acknowledges support from the European Research council (ERC-717001) and from the Netherlands Research Council NWO (016.VIDI.189.162). P.H. Johansson acknowledges the support from the European Research Council (ERC-818930). S. Toonen acknowledges support from the Netherlands Research Council NWO (VENI 639.041.645 Grants) C. Unal is supported by European Structural and Investment Funds and the Czech Ministry of Education, Youth and Sports (Project CoGraDS - CZ.02.1.01/0.0/0.0/15_003/0000437). S. Chaty acknowledges the LabEx UnivEarthS for the funding of Interface project I10 “From binary evolution towards merging of compact objects”. A. De Rosa acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.O E. Berti is supported by NSF Grants No. PHY-1912550 and AST-2006538, NASA ATP Grants No. 17-ATP17-0225 and 19-ATP19-0051, NSF-XSEDE Grant No. PHY-090003, and NSF Grant PHY-20043. D. Gerosa is supported by European Union’s H2020 ERC Starting Grant No. 945155–GWmining, Leverhulme Trust Grant No. RPG-2019-350 and Royal Society Grant No. RGS-R2-202004. T. Bogdanovic acknowledges support by the NASA award No. 80NSSC19K0319 and by the NSF award AST-1908042. D. Porquet acknowledges funding support from CNES. C. Danielski acknowledges financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award to the Instituto de Astrofísica de Andalucía (SEV-2017-0709) B.L. Davis acknowledges support from Tamkeen under the NYU Abu Dhabi Research Institute Grant CAP3. F. Pacucci acknowledges support from a Clay Fellowship by the SAO and from the Black Hole Initiative, which is funded by grants from the John Templeton Foundation and the Gordon and Betty Moore Foundation. A.J. Ruiter acknowledges support from the Australian Research Council Future Fellowship Grant FT170100243. V. Paschalidis is supported by NSF Grant PHY-1912619 and NASA Grant 80NSSC20K1542 to the University of Arizona, and NSF-XSEDE Grant TG-PHY190020. D. Haggard acknowledges support from the NSERC Discovery Grant and Canada Research Chairs programs, and the Bob Wares Science Innovation Prospectors Fund. M. Toscani acknowledges European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant Agreement No. 823823 (RISE DUSTBUSTERS project) and COST Action CA16104 - Gravitational waves, black holes and fundamental physics, supported by COST (European Cooperation in Science and Technology). M. Chruslinska, A. Istrate and G. Nelemans acknowledge support from Netherlands Research Council NWO. T. Fragos and S. Bavera acknowledge support from a Swiss National Science Foundation Professorship Grant (project numbers PP00P2_176868 and PP00P2_211006)., With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).

Published
2023

5. Astrophysics with the Laser Interferometer Space Antenna

Author

Amaro-Seoane, Pau, Andrews, Jeff, Sedda, Manuel Arca, Askar, Abbas, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stéphane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katie, Capelo, Pedro R., Caramete, Laurentiu, Catorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ross, Colpi, Monica, D'Orazio, Daniela, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriakos, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Fragkos, Tassos, Fryer, Chris, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul J., Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Tomas, Kokkotas, Kostas, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thomas, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Tomas, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Stefan, Mayer, Lucio, McGee, Sean, McKernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S., Nelemans, Gijs, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileios, Pfister, Hugo, Porquet, Delphine, Quenby, John, Röpke, Fritz, Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Rafaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlos, Stone, Nick, Suvorov, Arthur, Tamanini, Nicola, Tamfal, Tomas, Tauris, Thomas, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonios, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Rivera, Alexander Bonilla, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O'Shaughnessy, Richard, Zwart, Simon Portegies, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, Vigna-Gómez, Alejandro, Amaro-Seoane, Pau, Andrews, Jeff, Sedda, Manuel Arca, Askar, Abbas, Balasov, Razvan, Bartos, Imre, Bavera, Simone S., Bellovary, Jillian, Berry, Christopher P. L., Berti, Emanuele, Bianchi, Stefano, Blecha, Laura, Blondin, Stéphane, Bogdanović, Tamara, Boissier, Samuel, Bonetti, Matteo, Bonoli, Silvia, Bortolas, Elisa, Breivik, Katie, Capelo, Pedro R., Caramete, Laurentiu, Catorini, Federico, Charisi, Maria, Chaty, Sylvain, Chen, Xian, Chruślińska, Martyna, Chua, Alvin J. K., Church, Ross, Colpi, Monica, D'Orazio, Daniela, Danielski, Camilla, Davies, Melvyn B., Dayal, Pratika, De Rosa, Alessandra, Derdzinski, Andrea, Destounis, Kyriakos, Dotti, Massimo, Duţan, Ioana, Dvorkin, Irina, Fabj, Gaia, Foglizzo, Thierry, Ford, Saavik, Fouvry, Jean-Baptiste, Fragkos, Tassos, Fryer, Chris, Gaspari, Massimo, Gerosa, Davide, Graziani, Luca, Groot, Paul J., Habouzit, Melanie, Haggard, Daryl, Haiman, Zoltan, Han, Wen-Biao, Istrate, Alina, Johansson, Peter H., Khan, Fazeel Mahmood, Kimpson, Tomas, Kokkotas, Kostas, Kong, Albert, Korol, Valeriya, Kremer, Kyle, Kupfer, Thomas, Lamberts, Astrid, Larson, Shane, Lau, Mike, Liu, Dongliang, Lloyd-Ronning, Nicole, Lodato, Giuseppe, Lupi, Alessandro, Ma, Chung-Pei, Maccarone, Tomas, Mandel, Ilya, Mangiagli, Alberto, Mapelli, Michela, Mathis, Stefan, Mayer, Lucio, McGee, Sean, McKernan, Berry, Miller, M. Coleman, Mota, David F., Mumpower, Matthew, Nasim, Syeda S., Nelemans, Gijs, Noble, Scott, Pacucci, Fabio, Panessa, Francesca, Paschalidis, Vasileios, Pfister, Hugo, Porquet, Delphine, Quenby, John, Röpke, Fritz, Regan, John, Rosswog, Stephan, Ruiter, Ashley, Ruiz, Milton, Runnoe, Jessie, Schneider, Rafaella, Schnittman, Jeremy, Secunda, Amy, Sesana, Alberto, Seto, Naoki, Shao, Lijing, Shapiro, Stuart, Sopuerta, Carlos, Stone, Nick, Suvorov, Arthur, Tamanini, Nicola, Tamfal, Tomas, Tauris, Thomas, Temmink, Karel, Tomsick, John, Toonen, Silvia, Torres-Orjuela, Alejandro, Toscani, Martina, Tsokaros, Antonios, Unal, Caner, Vázquez-Aceves, Verónica, Valiante, Rosa, van Putten, Maurice, van Roestel, Jan, Vignali, Christian, Volonteri, Marta, Wu, Kinwah, Younsi, Ziri, Yu, Shenghua, Zane, Silvia, Zwick, Lorenz, Antonini, Fabio, Baibhav, Vishal, Barausse, Enrico, Rivera, Alexander Bonilla, Branchesi, Marica, Branduardi-Raymont, Graziella, Burdge, Kevin, Chakraborty, Srija, Cuadra, Jorge, Dage, Kristen, Davis, Benjamin, de Mink, Selma E., Decarli, Roberto, Doneva, Daniela, Escoffier, Stephanie, Gandhi, Poshak, Haardt, Francesco, Lousto, Carlos O., Nissanke, Samaya, Nordhaus, Jason, O'Shaughnessy, Richard, Zwart, Simon Portegies, Pound, Adam, Schussler, Fabian, Sergijenko, Olga, Spallicci, Alessandro, Vernieri, Daniele, and Vigna-Gómez, Alejandro

Abstract

Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy as it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and other space-based instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA's first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed: ultra-compact stellar-mass binaries, massive black hole binaries, and extreme or intermediate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help make progress in the different areas. New research avenues that LISA itself, or its joint exploitation with studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe., Comment: submitted to Living Reviews In Relativity

Published
2022

6. Multi-messenger astrophysics with THESEUS in the 2030s

Author

Ciolfi, Riccardo Stratta, Giulia Branchesi, Marica Gendre, Bruce Grimm, Stefan Harms, Jan Lamb, Gavin Paul and Martin-Carrillo, Antonio McCann, Ayden Oganesyan, Gor and Palazzi, Eliana Ronchini, Samuele Rossi, Andrea Salafia, Om Sharan Salmon, Lana Ascenzi, Stefano Capone, Antonio and Celli, Silvia Dall'Osso, Simone Di Palma, Irene Fasano, Michela Fermani, Paolo Guetta, Dafne Hanlon, Lorraine and Howell, Eric Paltani, Stephane Rezzolla, Luciano and Vinciguerra, Serena Zegarelli, Angela Amati, Lorenzo Blain, Andrew Bozzo, Enrico Chaty, Sylvain D'Avanzo, Paolo De Pasquale, FnmMassimiliano Dereli-Begue, Husne Ghirlanda, Giancarlo Gomboc, Andreja Gotz, Diego Horvath, Istvan and Hudec, Rene Izzo, Luca Le Floch, Emeric Li, Liang Longo, Francesco Komossa, S. Kong, Albert K. H. Mereghetti, Sandro and Mignani, Roberto Nathanail, Antonios O'Brien, Paul T. and Osborne, Julian P. Pe'er, Asaf Piranomonte, Silvia Rosati, Piero Savaglio, Sandra Schussler, Fabian Sergijenko, Olga and Shao, Lijing Tanvir, Nial Turriziani, Sara Urata, Yuji and van Putten, Maurice Vergani, Susanna Zane, Silvia Zhang, Bing

Abstract

Multi-messenger astrophysics is becoming a major avenue to explore the Universe, with the potential to span a vast range of redshifts. The growing synergies between different probes is opening new frontiers, which promise profound insights into several aspects of fundamental physics and cosmology. In this context, THESEUS will play a central role during the 2030s in detecting and localizing the electromagnetic counterparts of gravitational wave and neutrino sources that the unprecedented sensitivity of next generation detectors will discover at much higher rates than the present. Here, we review the most important target signals from multi-messenger sources that THESEUS will be able to detect and characterize, discussing detection rate expectations and scientific impact.

Published
2021

7. Multi-messenger astrophysics with THESEUS in the 2030s

Author

Ciolfi, Riccardo, Stratta, Giulia, Branchesi, Marica, Gendre, Bruce, Grimm, Stefan, Harms, Jan, Lamb, Gavin Paul, Martin-Carrillo, Antonio, McCann, Ayden, Oganesyan, Gor, Palazzi, Eliana, Ronchini, Samuele, Rossi, Andrea, Salafia, Om Sharan, Salmon, Lana, Ascenzi, Stefano, Capone, Antonio, Celli, Silvia, Dall'Osso, Simone, Di Palma, Irene, Fasano, Michela, Fermani, Paolo, Guetta, Dafne, Hanlon, Lorraine, Howell, Eric, Paltani, Stephane, Rezzolla, Luciano, Vinciguerra, Serena, Zegarelli, Angela, Amati, Lorenzo, Blain, Andrew, Bozzo, Enrico, Chaty, Sylvain, D'Avanzo, Paolo, De Pasquale, FnmMassimiliano, Dereli-Begue, Husne, Ghirlanda, Giancarlo, Gomboc, Andreja, Gotz, Diego, Horvath, Istvan, Hudec, Rene, Izzo, Luca, Le Floch, Emeric, Li, Liang, Longo, Francesco, Komossa, S., Kong, Albert K. H., Mereghetti, Sandro, Mignani, Roberto, Nathanail, Antonios, O'Brien, Paul T., Osborne, Julian P., Pe'er, Asaf, Piranomonte, Silvia, Rosati, Piero, Savaglio, Sandra, Schussler, Fabian, Sergijenko, Olga, Shao, Lijing, Tanvir, Nial, Turriziani, Sara, Urata, Yuji, van Putten, Maurice, Vergani, Susanna, Zane, Silvia, Zhang, Bing, Ciolfi, Riccardo, Stratta, Giulia, Branchesi, Marica, Gendre, Bruce, Grimm, Stefan, Harms, Jan, Lamb, Gavin Paul, Martin-Carrillo, Antonio, McCann, Ayden, Oganesyan, Gor, Palazzi, Eliana, Ronchini, Samuele, Rossi, Andrea, Salafia, Om Sharan, Salmon, Lana, Ascenzi, Stefano, Capone, Antonio, Celli, Silvia, Dall'Osso, Simone, Di Palma, Irene, Fasano, Michela, Fermani, Paolo, Guetta, Dafne, Hanlon, Lorraine, Howell, Eric, Paltani, Stephane, Rezzolla, Luciano, Vinciguerra, Serena, Zegarelli, Angela, Amati, Lorenzo, Blain, Andrew, Bozzo, Enrico, Chaty, Sylvain, D'Avanzo, Paolo, De Pasquale, FnmMassimiliano, Dereli-Begue, Husne, Ghirlanda, Giancarlo, Gomboc, Andreja, Gotz, Diego, Horvath, Istvan, Hudec, Rene, Izzo, Luca, Le Floch, Emeric, Li, Liang, Longo, Francesco, Komossa, S., Kong, Albert K. H., Mereghetti, Sandro, Mignani, Roberto, Nathanail, Antonios, O'Brien, Paul T., Osborne, Julian P., Pe'er, Asaf, Piranomonte, Silvia, Rosati, Piero, Savaglio, Sandra, Schussler, Fabian, Sergijenko, Olga, Shao, Lijing, Tanvir, Nial, Turriziani, Sara, Urata, Yuji, van Putten, Maurice, Vergani, Susanna, Zane, Silvia, and Zhang, Bing

Abstract

Multi-messenger astrophysics is becoming a major avenue to explore the Universe, with the potential to span a vast range of redshifts. The growing synergies between different probes is opening new frontiers, which promise profound insights into several aspects of fundamental physics and cosmology. In this context, THESEUS will play a central role during the 2030s in detecting and localizing the electromagnetic counterparts of gravitational wave and neutrino sources that the unprecedented sensitivity of next generation detectors will discover at much higher rates than the present. Here, we review the most important target signals from multi-messenger sources that THESEUS will be able to detect and characterize, discussing detection rate expectations and scientific impact.

Published
2021

8. The Giant Radio Array for Neutrino Detection (GRAND):Science and design

Author

Alvarez-Muniz, Jaime, Batista, Rafael Alves, Balagopal, Aswathi, Bolmont, Julien, Bustamante, Mauricio, Carvalho, Washington, Charrier, Didier, Cognard, Ismael, Decoene, Valentin, Denton, Peter B., De Jong, Sijbrand, De Vries, Krijn D., Engel, Ralph, Fang, Ke, Finley, Chad, Gabici, Stefano, Gou, QuanBu, Gu, JunHua, Guepin, Claire, Hu, HongBo, Huang, Yan, Kotera, Kumiko, Le Coz, Sandra, Lenain, Jean-Philippe, Lu, GuoLiang, Martineau-Huynh, Olivier, Mostafa, Miguel, Mottez, Fabrice, Murase, Kohta, Niess, Valentin, Oikonomou, Foteini, Pierog, Tanguy, Qian, XiangLi, Qin, Bo, Ran, Duan, Renault-Tinacci, Nicolas, Roth, Markus, Schroeder, Frank G., Schussler, Fabian, Tasse, Cyril, Timmermans, Charles, Tueros, Matias, Wu, XiangPing, Zarka, Philippe, Zech, Andreas, Zhang, B. Theodore, Zhang, JianLi, Zhang, Yi, Zheng, Qian, Zilles, Anne, Alvarez-Muniz, Jaime, Batista, Rafael Alves, Balagopal, Aswathi, Bolmont, Julien, Bustamante, Mauricio, Carvalho, Washington, Charrier, Didier, Cognard, Ismael, Decoene, Valentin, Denton, Peter B., De Jong, Sijbrand, De Vries, Krijn D., Engel, Ralph, Fang, Ke, Finley, Chad, Gabici, Stefano, Gou, QuanBu, Gu, JunHua, Guepin, Claire, Hu, HongBo, Huang, Yan, Kotera, Kumiko, Le Coz, Sandra, Lenain, Jean-Philippe, Lu, GuoLiang, Martineau-Huynh, Olivier, Mostafa, Miguel, Mottez, Fabrice, Murase, Kohta, Niess, Valentin, Oikonomou, Foteini, Pierog, Tanguy, Qian, XiangLi, Qin, Bo, Ran, Duan, Renault-Tinacci, Nicolas, Roth, Markus, Schroeder, Frank G., Schussler, Fabian, Tasse, Cyril, Timmermans, Charles, Tueros, Matias, Wu, XiangPing, Zarka, Philippe, Zech, Andreas, Zhang, B. Theodore, Zhang, JianLi, Zhang, Yi, Zheng, Qian, and Zilles, Anne

Abstract

The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km(2). A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND.

Published
2020

9. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

Author

Tamburini, Christian, Canals, Miquel, Durrieu De Madron, Xavier, Houpert, Loic, Lefevre, Dominique, Martini, Séverine, D'Ortenzio, Fabrizio, Robert, Anne, Testor, Pierre, Aguilar, Juan Antonio, Al Samarai, Imen, Albert, Arnaud, Andre, Michel, Anghinolfi, Marco, Anton, Gisela, Anvar, Shebli, Ardid, Miguel, Assis Jesus, Ana Carolina, Astraatmadja, Tri L., Aubert, Jean-jacques, Baret, Bruny, Basa, Stephane, Bertin, Vincent, Biagi, Simone, Bigi, Armando, Bigongiari, Ciro, Bogazzi, Claudio, Bou-cabo, Manuel, Bouhou, Boutayeb, Bouwhuis, Mieke C., Brunner, Jurgen, Busto, Jose, Camarena, Francisco, Capone, Antonio, Carloganu, Christina, Carminati, Giada, Carr, John, Cecchini, Stefano, Charif, Ziad, Charvis, Philippe, Chiarusi, Tommaso, Circella, Marco, Coniglione, Rosa, Costantini, Heide, Coyle, Paschal, Curtil, Christian, Decowski, Patrick, Dekeyser, Ivan, Deschamps, Anne, Donzaud, Corinne, Dornic, Damien, Dorosti, Hasankiadeh Q., Drouhin, Doriane, Eberl, Thomas, Emanuele, Umberto, Ernenwein, Jean-pierre, Escoffier, Stephanie, Fermani, Paolo, Ferri, Marcelino, Flaminio, Vincenzo, Folger, Florian, Fritsch, Ulf, Fuda, Jean-luc, Galata, Salvatore, Gay, Pascal, Giacomelli, Giorgio, Giordano, Valentina, Gomez-gonzalez, Juan-pablo, Graf, Kay, Guillard, Goulven, Halladjian, Garadeb, Hallewell, Gregory, Van Haren, Hans, Hartman, Joris, Heijboer, Aart J., Hello, Yann, Hernandez-rey, Juan Jose, Herold, Bjoern, Hossl, Jurgen, Hsu, Ching-cheng, De Jong, Marteen, Kadler, Matthias, Kalekin, Oleg, Kappes, Alexander, Katz, Uli, Kavatsyuk, Oksana, Kooijman, Paul, Kopper, Claudio, Kouchner, Antoine, Kreykenbohm, Ingo, Kulikovskiy, Vladimir, Lahmann, Robert, Lamare, Patrick, Larosa, Giuseppina, Lattuada, Dario, Lim, Gordon, Lo Presti, Domenico, Loehner, Herbert, Loucatos, Sotiris, Mangano, Salvatore, Marcelin, Michel, Margiotta, Annarita, Martinez-mora, Juan Antonio, Meli, Athina, Montaruli, Teresa, Moscoso, Luciano, Motz, Holger, Neff, Max, Nezri, Emmanuel, Palioselitis, Dimitris, Pavalas, Gabriela E., Payet, Kevin, Payre, Patrice, Petrovic, Jelena, Piattelli, Paolo, Picot-clemente, Nicolas, Popa, Vlad, Pradier, Thierry, Presani, Eleonora, Racca, Chantal, Reed, Corey, Riccobene, Giorgio, Richardt, Carsten, Richter, Roland, Riviere, Colas, Roensch, Kathrin, Rostovtsev, Andrei, Ruiz-rivas, Joaquin, Rujoiu, Marius, Russo, Valerio G., Salesa, Francisco, Sanchez-losa, Augustin, Sapienza, Piera, Schock, Friederike, Schuller, Jean-pierre, Schussler, Fabian, Shanidze, Rezo, Simeone, Francesco, Spies, Andreas, Spurio, Maurizio, Steijger, Jos J. M., Stolarczyk, Thierry, Taiuti, Mauro G. F., Toscano, Simona, Vallage, Bertrand, Van Elewyck, Veronique, Vannoni, Giulia, Vecchi, Manuela, Vernin, Pascal, Wijnker, Guus, Wilms, Jorn, De Wolf, Els, Yepes, Harold, Zaborov, Dmitry, Zornoza, Juan De Dios, Zuniga, Juan, Tamburini, Christian, Canals, Miquel, Durrieu De Madron, Xavier, Houpert, Loic, Lefevre, Dominique, Martini, Séverine, D'Ortenzio, Fabrizio, Robert, Anne, Testor, Pierre, Aguilar, Juan Antonio, Al Samarai, Imen, Albert, Arnaud, Andre, Michel, Anghinolfi, Marco, Anton, Gisela, Anvar, Shebli, Ardid, Miguel, Assis Jesus, Ana Carolina, Astraatmadja, Tri L., Aubert, Jean-jacques, Baret, Bruny, Basa, Stephane, Bertin, Vincent, Biagi, Simone, Bigi, Armando, Bigongiari, Ciro, Bogazzi, Claudio, Bou-cabo, Manuel, Bouhou, Boutayeb, Bouwhuis, Mieke C., Brunner, Jurgen, Busto, Jose, Camarena, Francisco, Capone, Antonio, Carloganu, Christina, Carminati, Giada, Carr, John, Cecchini, Stefano, Charif, Ziad, Charvis, Philippe, Chiarusi, Tommaso, Circella, Marco, Coniglione, Rosa, Costantini, Heide, Coyle, Paschal, Curtil, Christian, Decowski, Patrick, Dekeyser, Ivan, Deschamps, Anne, Donzaud, Corinne, Dornic, Damien, Dorosti, Hasankiadeh Q., Drouhin, Doriane, Eberl, Thomas, Emanuele, Umberto, Ernenwein, Jean-pierre, Escoffier, Stephanie, Fermani, Paolo, Ferri, Marcelino, Flaminio, Vincenzo, Folger, Florian, Fritsch, Ulf, Fuda, Jean-luc, Galata, Salvatore, Gay, Pascal, Giacomelli, Giorgio, Giordano, Valentina, Gomez-gonzalez, Juan-pablo, Graf, Kay, Guillard, Goulven, Halladjian, Garadeb, Hallewell, Gregory, Van Haren, Hans, Hartman, Joris, Heijboer, Aart J., Hello, Yann, Hernandez-rey, Juan Jose, Herold, Bjoern, Hossl, Jurgen, Hsu, Ching-cheng, De Jong, Marteen, Kadler, Matthias, Kalekin, Oleg, Kappes, Alexander, Katz, Uli, Kavatsyuk, Oksana, Kooijman, Paul, Kopper, Claudio, Kouchner, Antoine, Kreykenbohm, Ingo, Kulikovskiy, Vladimir, Lahmann, Robert, Lamare, Patrick, Larosa, Giuseppina, Lattuada, Dario, Lim, Gordon, Lo Presti, Domenico, Loehner, Herbert, Loucatos, Sotiris, Mangano, Salvatore, Marcelin, Michel, Margiotta, Annarita, Martinez-mora, Juan Antonio, Meli, Athina, Montaruli, Teresa, Moscoso, Luciano, Motz, Holger, Neff, Max, Nezri, Emmanuel, Palioselitis, Dimitris, Pavalas, Gabriela E., Payet, Kevin, Payre, Patrice, Petrovic, Jelena, Piattelli, Paolo, Picot-clemente, Nicolas, Popa, Vlad, Pradier, Thierry, Presani, Eleonora, Racca, Chantal, Reed, Corey, Riccobene, Giorgio, Richardt, Carsten, Richter, Roland, Riviere, Colas, Roensch, Kathrin, Rostovtsev, Andrei, Ruiz-rivas, Joaquin, Rujoiu, Marius, Russo, Valerio G., Salesa, Francisco, Sanchez-losa, Augustin, Sapienza, Piera, Schock, Friederike, Schuller, Jean-pierre, Schussler, Fabian, Shanidze, Rezo, Simeone, Francesco, Spies, Andreas, Spurio, Maurizio, Steijger, Jos J. M., Stolarczyk, Thierry, Taiuti, Mauro G. F., Toscano, Simona, Vallage, Bertrand, Van Elewyck, Veronique, Vannoni, Giulia, Vecchi, Manuela, Vernin, Pascal, Wijnker, Guus, Wilms, Jorn, De Wolf, Els, Yepes, Harold, Zaborov, Dmitry, Zornoza, Juan De Dios, and Zuniga, Juan

Abstract

The deep ocean is the largest and least known ecosystem on Earth. It hosts numerous pelagic organisms, most of which are able to emit light. Here we present a unique data set consisting of a 2.5-year long record of light emission by deep-sea pelagic organisms, measured from December 2007 to June 2010 at the ANTARES underwater neutrino telescope in the deep NW Mediterranean Sea, jointly with synchronous hydrological records. This is the longest continuous time-series of deep-sea bioluminescence ever recorded. Our record reveals several weeks long, seasonal bioluminescence blooms with light intensity up to two orders of magnitude higher than background values, which correlate to changes in the properties of deep waters. Such changes are triggered by the winter cooling and evaporation experienced by the upper ocean layer in the Gulf of Lion that leads to the formation and subsequent sinking of dense water through a process known as "open-sea convection". It episodically renews the deep water of the study area and conveys fresh organic matter that fuels the deep ecosystems. Luminous bacteria most likely are the main contributors to the observed deep-sea bioluminescence blooms. Our observations demonstrate a consistent and rapid connection between deep open-sea convection and bathypelagic biological activity, as expressed by bioluminescence. In a setting where dense water formation events are likely to decline under global warming scenarios enhancing ocean stratification, in situ observatories become essential as environmental sentinels for the monitoring and understanding of deep-sea ecosystem shifts.

Published
2013
Full Text
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10. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

Author

Roberts, John Murray, Tamburini, Christian, Canals, Miquel, Durrieu de Madron, Xavier, Houpert, Loïc, Lefèvre, Dominique, Martini, Séverine, D'Ortenzio, Fabrizio, Robert, Anne, Testor, Pierre, Aguilar, Juan Antonio, Samarai, Imen Al, Albert, Arnaud, André, Michel, Anghinolfi, Marco, Anton, Gisela, Anvar, Shebli, Ardid, Miguel, Jesus, Ana Carolina Assis, Astraatmadja, Tri L., Aubert, Jean-Jacques, Baret, Bruny, Basa, Stéphane, Bertin, Vincent, Biagi, Simone, Bigi, Armando, Bigongiari, Ciro, Bogazzi, Claudio, Bou-Cabo, Manuel, Bouhou, Boutayeb, Bouwhuis, Mieke C., Brunner, Jurgen, Busto, José, Camarena, Francisco, Capone, Antonio, Cârloganu, Christina, Carminati, Giada, Carr, John, Cecchini, Stefano, Charif, Ziad, Charvis, Philippe, Chiarusi, Tommaso, Circella, Marco, Coniglione, Rosa, Costantini, Heide, Coyle, Paschal, Curtil, Christian, Decowski, Patrick, Dekeyser, Ivan, Deschamps, Anne, Donzaud, Corinne, Dornic, Damien, Dorosti, Hasankiadeh Q., Drouhin, Doriane, Eberl, Thomas, Emanuele, Umberto, Ernenwein, Jean-Pierre, Escoffier, Stéphanie, Fermani, Paolo, Ferri, Marcelino, Flaminio, Vincenzo, Folger, Florian, Fritsch, Ulf, Fuda, Jean-Luc, Galatà, Salvatore, Gay, Pascal, Giacomelli, Giorgio, Giordano, Valentina, Gómez-González, Juan-Pablo, Graf, Kay, Guillard, Goulven, Halladjian, Garadeb, Hallewell, Gregory, van Haren, Hans, Hartman, Joris, Heijboer, Aart J., Hello, Yann, Hernández-Rey, Juan Jose, Herold, Bjoern, Hößl, Jurgen, Hsu, Ching-Cheng, de Jong, Marteen, Kadler, Matthias, Kalekin, Oleg, Kappes, Alexander, Katz, Uli, Kavatsyuk, Oksana, Kooijman, Paul, Kopper, Claudio, Kouchner, Antoine, Kreykenbohm, Ingo, Kulikovskiy, Vladimir, Lahmann, Robert, Lamare, Patrick, Larosa, Giuseppina, Lattuada, Dario, Lim, Gordon, Presti, Domenico Lo, Loehner, Herbert, Loucatos, Sotiris, Mangano, Salvatore, Marcelin, Michel, Margiotta, Annarita, Martinez-Mora, Juan Antonio, Meli, Athina, Montaruli, Teresa, Moscoso, Luciano, Motz, Holger, Neff, Max, Nezri, Emma nuel, Palioselitis, Dimitris, Păvălaş, Gabriela E., Payet, Kevin, Payre, Patrice, Petrovic, Jelena, Piattelli, Paolo, Picot-Clemente, Nicolas, Popa, Vlad, Pradier, Thierry, Presani, Eleonora, Racca, Chantal, Reed, Corey, Riccobene, Giorgio, Richardt, Carsten, Richter, Roland, Rivière, Colas, Roensch, Kathrin, Rostovtsev, Andrei, Ruiz-Rivas, Joaquin, Rujoiu, Marius, Russo, Valerio G., Salesa, Francisco, Sánchez-Losa, Augustin, Sapienza, Piera, Schöck, Friederike, Schuller, Jean-Pierre, Schussler, Fabian, Shanidze, Rezo, Simeone, Francesco, Spies, Andreas, Spurio, Maurizio, Steijger, Jos J. M., Stolarczyk, Thierry, Taiuti, Mauro G. F., Toscano, Simona, Vallage, Bertrand, Van Elewyck, Véronique, Vannoni, Giulia, Vecchi, Manuela, Vernin, Pascal, Wijnker, Guus, Wilms, Jorn, de Wolf, Els, Yepes, Harold, Zaborov, Dmitry, De Dios Zornoza, Juan, Zúñiga, Juan, Roberts, John Murray, Tamburini, Christian, Canals, Miquel, Durrieu de Madron, Xavier, Houpert, Loïc, Lefèvre, Dominique, Martini, Séverine, D'Ortenzio, Fabrizio, Robert, Anne, Testor, Pierre, Aguilar, Juan Antonio, Samarai, Imen Al, Albert, Arnaud, André, Michel, Anghinolfi, Marco, Anton, Gisela, Anvar, Shebli, Ardid, Miguel, Jesus, Ana Carolina Assis, Astraatmadja, Tri L., Aubert, Jean-Jacques, Baret, Bruny, Basa, Stéphane, Bertin, Vincent, Biagi, Simone, Bigi, Armando, Bigongiari, Ciro, Bogazzi, Claudio, Bou-Cabo, Manuel, Bouhou, Boutayeb, Bouwhuis, Mieke C., Brunner, Jurgen, Busto, José, Camarena, Francisco, Capone, Antonio, Cârloganu, Christina, Carminati, Giada, Carr, John, Cecchini, Stefano, Charif, Ziad, Charvis, Philippe, Chiarusi, Tommaso, Circella, Marco, Coniglione, Rosa, Costantini, Heide, Coyle, Paschal, Curtil, Christian, Decowski, Patrick, Dekeyser, Ivan, Deschamps, Anne, Donzaud, Corinne, Dornic, Damien, Dorosti, Hasankiadeh Q., Drouhin, Doriane, Eberl, Thomas, Emanuele, Umberto, Ernenwein, Jean-Pierre, Escoffier, Stéphanie, Fermani, Paolo, Ferri, Marcelino, Flaminio, Vincenzo, Folger, Florian, Fritsch, Ulf, Fuda, Jean-Luc, Galatà, Salvatore, Gay, Pascal, Giacomelli, Giorgio, Giordano, Valentina, Gómez-González, Juan-Pablo, Graf, Kay, Guillard, Goulven, Halladjian, Garadeb, Hallewell, Gregory, van Haren, Hans, Hartman, Joris, Heijboer, Aart J., Hello, Yann, Hernández-Rey, Juan Jose, Herold, Bjoern, Hößl, Jurgen, Hsu, Ching-Cheng, de Jong, Marteen, Kadler, Matthias, Kalekin, Oleg, Kappes, Alexander, Katz, Uli, Kavatsyuk, Oksana, Kooijman, Paul, Kopper, Claudio, Kouchner, Antoine, Kreykenbohm, Ingo, Kulikovskiy, Vladimir, Lahmann, Robert, Lamare, Patrick, Larosa, Giuseppina, Lattuada, Dario, Lim, Gordon, Presti, Domenico Lo, Loehner, Herbert, Loucatos, Sotiris, Mangano, Salvatore, Marcelin, Michel, Margiotta, Annarita, Martinez-Mora, Juan Antonio, Meli, Athina, Montaruli, Teresa, Moscoso, Luciano, Motz, Holger, Neff, Max, Nezri, Emma nuel, Palioselitis, Dimitris, Păvălaş, Gabriela E., Payet, Kevin, Payre, Patrice, Petrovic, Jelena, Piattelli, Paolo, Picot-Clemente, Nicolas, Popa, Vlad, Pradier, Thierry, Presani, Eleonora, Racca, Chantal, Reed, Corey, Riccobene, Giorgio, Richardt, Carsten, Richter, Roland, Rivière, Colas, Roensch, Kathrin, Rostovtsev, Andrei, Ruiz-Rivas, Joaquin, Rujoiu, Marius, Russo, Valerio G., Salesa, Francisco, Sánchez-Losa, Augustin, Sapienza, Piera, Schöck, Friederike, Schuller, Jean-Pierre, Schussler, Fabian, Shanidze, Rezo, Simeone, Francesco, Spies, Andreas, Spurio, Maurizio, Steijger, Jos J. M., Stolarczyk, Thierry, Taiuti, Mauro G. F., Toscano, Simona, Vallage, Bertrand, Van Elewyck, Véronique, Vannoni, Giulia, Vecchi, Manuela, Vernin, Pascal, Wijnker, Guus, Wilms, Jorn, de Wolf, Els, Yepes, Harold, Zaborov, Dmitry, De Dios Zornoza, Juan, and Zúñiga, Juan

Abstract

The deep ocean is the largest and least known ecosystem on Earth. It hosts numerous pelagic organisms, most of which are able to emit light. Here we present a unique data set consisting of a 2.5-year long record of light emission by deep-sea pelagic organisms, measured from December 2007 to June 2010 at the ANTARES underwater neutrino telescope in the deep NW Mediterranean Sea, jointly with synchronous hydrological records. This is the longest continuous time-series of deep-sea bioluminescence ever recorded. Our record reveals several weeks long, seasonal bioluminescence blooms with light intensity up to two orders of magnitude higher than background values, which correlate to changes in the properties of deep waters. Such changes are triggered by the winter cooling and evaporation experienced by the upper ocean layer in the Gulf of Lion that leads to the formation and subsequent sinking of dense water through a process known as “open-sea convection”. It episodically renews the deep water of the study area and conveys fresh organic matter that fuels the deep ecosystems. Luminous bacteria most likely are the main contributors to the observed deep-sea bioluminescence blooms. Our observations demonstrate a consistent and rapid connection between deep open-sea convection and bathypelagic biological activity, as expressed by bioluminescence. In a setting where dense water formation events are likely to decline under global warming scenarios enhancing ocean stratification, in situ observatories become essential as environmental sentinels for the monitoring and understanding of deep-sea ecosystem shifts.

Published
2013

11. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

Author

Tamburini, Christian, primary, Canals, Miquel, additional, Durrieu de Madron, Xavier, additional, Houpert, Loïc, additional, Lefèvre, Dominique, additional, Martini, Séverine, additional, D'Ortenzio, Fabrizio, additional, Robert, Anne, additional, Testor, Pierre, additional, Aguilar, Juan Antonio, additional, Samarai, Imen Al, additional, Albert, Arnaud, additional, André, Michel, additional, Anghinolfi, Marco, additional, Anton, Gisela, additional, Anvar, Shebli, additional, Ardid, Miguel, additional, Jesus, Ana Carolina Assis, additional, Astraatmadja, Tri L., additional, Aubert, Jean-Jacques, additional, Baret, Bruny, additional, Basa, Stéphane, additional, Bertin, Vincent, additional, Biagi, Simone, additional, Bigi, Armando, additional, Bigongiari, Ciro, additional, Bogazzi, Claudio, additional, Bou-Cabo, Manuel, additional, Bouhou, Boutayeb, additional, Bouwhuis, Mieke C., additional, Brunner, Jurgen, additional, Busto, José, additional, Camarena, Francisco, additional, Capone, Antonio, additional, Cârloganu, Christina, additional, Carminati, Giada, additional, Carr, John, additional, Cecchini, Stefano, additional, Charif, Ziad, additional, Charvis, Philippe, additional, Chiarusi, Tommaso, additional, Circella, Marco, additional, Coniglione, Rosa, additional, Costantini, Heide, additional, Coyle, Paschal, additional, Curtil, Christian, additional, Decowski, Patrick, additional, Dekeyser, Ivan, additional, Deschamps, Anne, additional, Donzaud, Corinne, additional, Dornic, Damien, additional, Dorosti, Hasankiadeh Q., additional, Drouhin, Doriane, additional, Eberl, Thomas, additional, Emanuele, Umberto, additional, Ernenwein, Jean-Pierre, additional, Escoffier, Stéphanie, additional, Fermani, Paolo, additional, Ferri, Marcelino, additional, Flaminio, Vincenzo, additional, Folger, Florian, additional, Fritsch, Ulf, additional, Fuda, Jean-Luc, additional, Galatà, Salvatore, additional, Gay, Pascal, additional, Giacomelli, Giorgio, additional, Giordano, Valentina, additional, Gómez-González, Juan-Pablo, additional, Graf, Kay, additional, Guillard, Goulven, additional, Halladjian, Garadeb, additional, Hallewell, Gregory, additional, van Haren, Hans, additional, Hartman, Joris, additional, Heijboer, Aart J., additional, Hello, Yann, additional, Hernández-Rey, Juan Jose, additional, Herold, Bjoern, additional, Hößl, Jurgen, additional, Hsu, Ching-Cheng, additional, de Jong, Marteen, additional, Kadler, Matthias, additional, Kalekin, Oleg, additional, Kappes, Alexander, additional, Katz, Uli, additional, Kavatsyuk, Oksana, additional, Kooijman, Paul, additional, Kopper, Claudio, additional, Kouchner, Antoine, additional, Kreykenbohm, Ingo, additional, Kulikovskiy, Vladimir, additional, Lahmann, Robert, additional, Lamare, Patrick, additional, Larosa, Giuseppina, additional, Lattuada, Dario, additional, Lim, Gordon, additional, Presti, Domenico Lo, additional, Loehner, Herbert, additional, Loucatos, Sotiris, additional, Mangano, Salvatore, additional, Marcelin, Michel, additional, Margiotta, Annarita, additional, Martinez-Mora, Juan Antonio, additional, Meli, Athina, additional, Montaruli, Teresa, additional, Moscoso, Luciano, additional, Motz, Holger, additional, Neff, Max, additional, Nezri, Emma nuel, additional, Palioselitis, Dimitris, additional, Păvălaş, Gabriela E., additional, Payet, Kevin, additional, Payre, Patrice, additional, Petrovic, Jelena, additional, Piattelli, Paolo, additional, Picot-Clemente, Nicolas, additional, Popa, Vlad, additional, Pradier, Thierry, additional, Presani, Eleonora, additional, Racca, Chantal, additional, Reed, Corey, additional, Riccobene, Giorgio, additional, Richardt, Carsten, additional, Richter, Roland, additional, Rivière, Colas, additional, Roensch, Kathrin, additional, Rostovtsev, Andrei, additional, Ruiz-Rivas, Joaquin, additional, Rujoiu, Marius, additional, Russo, Valerio G., additional, Salesa, Francisco, additional, Sánchez-Losa, Augustin, additional, Sapienza, Piera, additional, Schöck, Friederike, additional, Schuller, Jean-Pierre, additional, Schussler, Fabian, additional, Shanidze, Rezo, additional, Simeone, Francesco, additional, Spies, Andreas, additional, Spurio, Maurizio, additional, Steijger, Jos J. M., additional, Stolarczyk, Thierry, additional, Taiuti, Mauro G. F., additional, Toscano, Simona, additional, Vallage, Bertrand, additional, Van Elewyck, Véronique, additional, Vannoni, Giulia, additional, Vecchi, Manuela, additional, Vernin, Pascal, additional, Wijnker, Guus, additional, Wilms, Jorn, additional, de Wolf, Els, additional, Yepes, Harold, additional, Zaborov, Dmitry, additional, De Dios Zornoza, Juan, additional, and Zúñiga, Juan, additional

Published
2013
Full Text
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12. Search for neutrinos from transient sources with the ANTARES telescope and optical follow-up observations

Author

Ageron, Michel, primary, Al Samarai, Imen, additional, Akerlof, Carl, additional, Basa, Stéphane, additional, Bertin, Vincent, additional, Boer, Michel, additional, Brunner, Juergen, additional, Busto, Jose, additional, Dornic, Damien, additional, Klotz, Alain, additional, Schussler, Fabian, additional, Vallage, Bertrand, additional, Vecchi, Manuela, additional, and Zheng, Weikang, additional

Published
2012
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13. Fission dynamics for capture reactions in 58,64ni + 208pb systems: New results in terms of thermal energy and neutron multiplicity correlated distributions

Author

Donadille, Laurent, Liatard, Eric, Désesquelles, Pierre, Bruandet, J.F. J.F., Farget, Fanny, Fayot, J., Perrin, G., Santos, De, Schussler, Fabian, Viano, J. B., Vignon, B., Benoit, Bénédicte, Hanappe, Francis, Stuttge, Louise, Rudolf, Gérard, Bilwes, B., Costa, G., Dorvaux, O., Guillaume, G., Huck, Alexander, Tomaśevič, S., Kozulin, E.M., Lazarev, Yu Y.A., Itkis, I.M., Itkis, Mikhail, Kondratiev, N.A., Oganessian, Yu.Ts., Litnevsky, L.A. L.A., Jokic, Stevan, Lecolley, François René, Lecolley, Jean François, Donadille, Laurent, Liatard, Eric, Désesquelles, Pierre, Bruandet, J.F. J.F., Farget, Fanny, Fayot, J., Perrin, G., Santos, De, Schussler, Fabian, Viano, J. B., Vignon, B., Benoit, Bénédicte, Hanappe, Francis, Stuttge, Louise, Rudolf, Gérard, Bilwes, B., Costa, G., Dorvaux, O., Guillaume, G., Huck, Alexander, Tomaśevič, S., Kozulin, E.M., Lazarev, Yu Y.A., Itkis, I.M., Itkis, Mikhail, Kondratiev, N.A., Oganessian, Yu.Ts., Litnevsky, L.A. L.A., Jokic, Stevan, Lecolley, François René, and Lecolley, Jean François

Abstract

The neutron multidetector DéMoN has been used to investigate the symmetric splitting dynamics in the reactions 58.64Ni + 208Pb with excitation energies ranging from 65 to 186 MeV for the composite system. An analysis based on the new backtracing technique has been applied on the neutron data to determine the two-dimensional correlations between the parent composite system initial thermal energy (EthCN) and the total neutron multiplicity (νtot), and between pre- and post-scission neutron multiplicities (νpre and νpost, respectively). The νpre distribution shape indicates the possible coexistence of fast-fission and fusion-fission for the system 58Ni + 208Pb (Ebeam = 8.86 A MeV). The analysis of the neutron multiplicities in the framework of the combined dynamical statistical model (CDSM) gives a reduced friction coefficient β = 23 ± 2512 × 1021 s-1, above the one-body dissipation limit. The corresponding fission time is τf = 40 ± 4620 × 10-21 s. © 1999 Elsevier Science B.V. All rights reserved., SCOPUS: ar.j, info:eu-repo/semantics/published

Published
1999

14. Relativistic jets in microquasars.

Author

RODRIGUEZ, JÉRÔME and SCHUSSLER, FABIAN

Subjects
*RADIO jets (Astrophysics), *QUASARS, *SYNCHROTRON radiation, *GRAVITATIONAL energy, *ACCRETION (Astrophysics)
Abstract

The article offers information on the violent jets which are the energy engines for the microquasars. Topics include that the \jets emit by synchrotron radiation and dominate as of the radio band; and discusses that the compacts jets are associated with states in which accretion is more regular and relatively inefficient as the gravitational energy is here redistributed in the jets rather than in radiative form.

Published
2019

16. Operations of and Future Plans for the Pierre Auger Observatory

Author

Abraham, Jorge Alberto, Abreu, Pedro, Aglietta, M., Aguirre, Carlos, Ahn, Eun-Joo, Allard, Denis, Allekotte, Ingo, Allen, Ronald J., Allison, Patrick, Alvarez-Muniz, Jaime, Ambrosio, Michelangelo, Anchordoqui, Luis Alfredo, Andringa, Sofia, Anzalone, Anna, Aramo, Carla, Arganda, E., Argiro, Stefano, Arisaka, Katsushi, Arneodo, F., Arqueros, Fernando, Asch, T., Asorey, Hernan, Assis, Pedro, Aublin, Julien, Ave, Maximo, Avila, Gualberto, Bacher, A., Backer, T., Badagnani, Daniel Omar, Barber, Kerridwen B., Barbosa, A. F., Barbosa, Henrique J. M., Barenthien, Norbert, Barroso, S. L. C., Baughman, Brian, Bauleo, Pablo Miguel, Beatty, James J., Beau, Tristan, Becker, Bernard Raymond, Becker, Karl-Heinz, Belletoile, Arnaud, Bellido, Jose Alfredo, Benzvi, Segev, Berat, Corinne, Bernardini, Paolo, Bertou, Xavier, Biermann, Peter L., Billoir, Pierre, Blanch, Oscar, Blanco, Francisco, Bleve, Carla, Blumer, Hans, Bohacova, Martina, Bollmann, E., Bolz, H., Bonifazi, Carla, Bonino, Raffaella, Borodai, N., Bracci, F., Brack, Jeffrey, Brogueira, P., Brown, William C., Bruijn, Ronald, Buchholz, Peter, Bueno, Antonio, Burton, R. E., Busca, Nicolas Guillermo, Caballero-Mora, Karen Salome, Camin, Daniel V., Caramete, L., Caruso, Rossella, Carvalho, Washington R., Castellina, Antonella, Castro-Tirado, A. J., Catalano, O., Cazon, Lorenzo, Cester, Rosanna, Chauvin, Joel, Chiavassa, A., Chinellato, Jose Augusto, Chou, Aaron S., Chudoba, Jiri, Chye, James D., Clark, Paul D. J., Clay, Roger William, Colombo, Eduardo, Conceicao, R., Connolly, Brian M., Contreras, Fernando, Coppens, Jose, Cordero-Cid, Adriana, Cordier, Alain, Cotti, Umberto, Coutu, Stephane, Covault, Corbin E., Creusot, Alexandre, Criss, Adrienne, Cronin, James Watson, Cuautle, J., Curutiu, A., Dagoret-Campagne, Sylvie, Dallier, Richard, Daudo, F., Daumiller, Kai, Dawson, Bruce R., Almeida, Rogerio Menezes, Domenico, Manlio, Donato, Cinzia, Jong, Sijbrand Jan, La Vega, G., Mello Junior, W. J. M., Mello Neto, Joao Ramos Torres, Mitri, Ivan, Souza, Vitor, Vries, K. D., Decerprit, G., Del Peral, Luis, Deligny, Olivier, Della Selva, Angelo, Delle Fratte, C., Dembinski, Hans, Di Giulio, Claudio, Diaz-Velez, J. C., Diep, P. N., Dobrigkeit, Carola, D Olivo, Juan Carlos, Dong, P. N., Dornic, Damien, Dorofeev, Alexei V., Costa Dos Anjos, Joao Carlos, Dova, Maria Teresa, D Urso, Domenico, Dutan, I., Duvernois, Michael A., Engel, Ralph, Erdmann, Martin Hans, Escobar, Carlos Ourivio, Etchegoyen, Alberto, Facal San Luis, Pedro, Falcke, Heino, Farrar, Glennys R., Fauth, Anderson C., Fazzini, N., Ferrer, Francesc, Ferrero, Armando, Fick, Brian E., Filevich, Alberto, Filipcic, Andrej, Fleck, Ivor, Fliescher, Stefan, Fonte, Roberto, Fracchiolla, Claudia E., Fraenkel, E. D., Fulgione, Walter, Gamarra, R. F., Gambetta, S., Garcia, Beatriz, Garcia-Gamez, Diego, Garcia-Pinto, D., Garrido, Xavier, Geenen, Heiko, Gelmini, Graciela B., Gemmeke, Hartmut, Ghia, Piera Luisa, Giaccari, Ugo, Gibbs, Kenneth, Giller, Maria, Gitto, J., Glass, Henry D., Goggin, Lisa M., Gold, Michael S., Golup, Geraldina T., Gomez Albarracin, F., Gomez Berisso, M., Gomez Vitale, P. F., Goncalves, Patricia, Goncalves Do Amaral, Marcia, Gonzalez, D., Gonzalez, J. G., Gora, Dariusz, Gorgi, A., Gouffon, Philippe H., Grashorn, Eric W., Grassi, V., Grebe, Stefan, Grigat, Marius, Grillo, Aurelio F., Grygar, Jiri, Guardincerri, Y., Guardone, Nunzio, Guerard, Carlos, Guarino, Francesco, Gumbsheimer, Rainer, Guedes, G. P., Gutierrez, J., Hague, J. D., Halenka, V., Hansen, P., Harari, Diego, Harmsma, Sybren, Hartmann, Steffen, Harton, John L., Haungs, Andreas, Healy, Matthew D., Hebbeker, Thomas, Hebrero, G., Heck, Dieter, Hojvat, Carlos F., Holmes, Vanessa Catherine, Homola, Piotr, Hofman, G., Hoerandel, Joerg R., Horneffer, A., Horvat, Matje, Hrabovsky, Miroslav, Hucker, H., Huege, Tim, Hussain, M., Iarlori, Marco, Insolia, Antonio, Ionita, F., Italiano, A., Jiraskova, S., Kaducak, Marc L., Kampert, Karl-Heinz, Karova, Tatiana, Kasper, Peter H., Kegl, B., Keilhauer, Bianca G., Kemp, Ernesto, Kern, H., Kieckhafer, Roger M., Klages, Hans O., Kleifges, Matthias, Kleinfeller, Jonny, Knapik, Robert, Knapp, Johannes, Koang, Dy-Holm, Kopmann, Andreas, Krieger, A., Kromer, O., Kruppke-Hansen, Daniel, Kuempel, Daniel, Kunka, Norbert, Kusenko, Alexander, La Rosa, Giovanni, Lachaud, C., Lago, B. L., Lautridou, Pascal, Leao, M. S. A. B., Lebrun, D., Lebrun, Paul L. G., Lee, Joong, Leigui Oliveira, Marcelo A., Lemiere, Anne, Letessier-Selvon, Antoine, Leuthold, Matthias J., Lhenry-Yvon, Isabelle, Lopez, Rebeca, Lopez Aguera, Angeles, Louedec, Karim, Lozano Bahilo, Julio, Lucero, A., Lyberis, H., Maccarone, Marie Concetta, Macolino, Carla, Maldera, Simone, Malek, Matthew Samir, Mandat, Dusan, Mantsch, Paul M., Marchetto, Flavio Pietro, Mariazzi, Analisa G., Maris, Ioana C., Marquez-Falcon, Hugo Raymundo, Martello, Daniele, Martineau-Huynh, O., Martinez Bravo, Oscar Mario, Mathes, Hermann-Josef, Matthews, J., Matthews, John A. J., Matthiae, Giorgio, Maurizio, Daniela, Mazur, Peter O., Mcewen, Megan, Mcneil, Roger Richard, Medina-Tanco, Gustavo A., Melissas, Maximilien, Melo, Diego G., Menichetti, Ezio A., Menshikov, Alexander, Meyhandan, Rishi, Micheletti, Maria Isabel, Miele, Gennaro, Miller, William, Miramonti, Lino, Mollerach, Silvia, Monasor, Maria, Monnier-Ragaigne, Delphine, Montanet, Francois, Morales, Benjamin Alejandro, Morello, C., Moreno, Juan Cruz, Morris, D. C., Mostafa, Miguel Alejandro, Moura, C. A., Mucchi, M., Mueller, S., Muller, M. A., Mussa, Roberto, Navarra, Gianni, Navarro, Jose Luis, Navas, Sergio, Necesal, P., Nellen, Lukas, Nerling, F., Newman-Holmes, Catherine, Newton, D., Nhung, P. T., Nicotra, Domenico, Nierstenhoefer, Nils, Nitz, David F., Nosek, Dalibor, Nozka, Libor, Nyklicek, M., Oehlschlager, J., Olinto, Angela V., Oliva, Pietro, Olmos-Gilbaja, Victor Manuel, Ortiz, Montserrat, Ortolani, Fabrizio, Osswald, B., Pacheco, N., Pakk Selmi-Dei, D., Palatka, Miroslav, Pallotta, J., Parente, Gonzalo, Parizot, Etienne, Parlati, S., Pastor, Sergio, Patel, M., Paul, Thomas Cantzon, Payet, Kevin, Pech, Miroslav, Pekala, J., Pepe, Iuri M., Perrone, Lorenzo, Pesce, R., Petermann, E., Petrera, Sergio, Petrinca, P., Petrolini, Alessandro, Petrov, Yuri V., Petrovic, J., Pfendner, C., Pichel, A., Piegaia, Ricardo, Pierog, Tanguy, Pimenta, Mario, Pinto, Teguayco, Pirronello, Valerio, Pisanti, Ofelia, Platino, M., Pochon, Jonathan, Ponce, Victor Hugo, Pontz, Michael, Pouryamout, J., Prado, Luis, Privitera, Paolo, Prouza, Michael, Quel, E. J., Raia, G., Rautenberg, Julian, Ravel, Olivier, Ravignani, Diego, Redondo, A., Reis, H. C., Reucroft, Stephen, Revenu, Benoit, Seixas Rezende, Fabio Antonio, Ridky, Jan, Riggi, Simone, Risse, Markus, Riviere, Christophe, Rizi, Vincenzo, Robledo, C., Roberts, M. D., Rodriguez-Fernandez, Gonzalo, Rodriguez Martino, Julio Cesar, Rodriguez Rojo, J., Rodriguez-Cabo, I., Rodriguez-Frias, M. Dolores, Ros, German, Rosado, Jaime, Rossler, T., Roth, Markus, Rouille-D Orfeuil, Benjamin, Roulet, Esteban, Rovero, Adrian C., Salamida, Francesco, Salina, Gaetano, Sanchez, Federico, Santander, Juan Marcos, Santo, C. E., Moura Santos, Edivaldo, Sarazin, Fred, Subir Sarkar, Sato, Ricardo, Scharf, Nils, Scherini, Viviana, Schieler, Harald, Schiffer, Peter, Schleif, G., Schmidt, A. A., Schmidt, Fabian, Schmidt, Talianna, Scholten, Olaf, Schoorlemmer, Harm, Schovancova, J., Schovanek, Petr, Schroeder, F., Schulte, Stephan, Schussler, Fabian, Schuster, David, Sciutto, Sergio J., Scuderi, Mario, Segreto, A., Semikoz, Dmitri V., Sequieros, G., Settimo, Mariangela, Shellard, Ronald Cintra, Sidelnik, Ivan, Siffert, Beatriz B., Smialkowski, Andrzej, Smida, Radomir, Smith, Andrew G. K., Smith, Ben E., Snow, Gregory R., Sommers, Paul D., Sorokin, J., Spinka, Harold M., Squartini, Ruben, Strazzeri, Elisabetta, Stutz, Anne, Suarez, F., Suomijarvi, Tiina, Supanitsky, A. D., Sutherland, Michael S., Swain, John D., Szadkowski, Zbigniew, Tamashiro, Alejandro Andres, Tamburro, Alessio, Tarutina, T., Tascau, Oana, Tcaciuc, Rodica, Tcherniakhovski, Denis, Thao, Nguyen Thi, Thomas, David, Ticona, R., Tiffenberg, Javier, Timmermans, Charles, Tkaczyk, Wieslaw, Todero Peixoto, C. J., Tome, Brigitte, Tonachini, Aurelio, Torres, I., Trapani, P., Travnicek, Petr, Tridapalli, Diogo B., Tristram, Gerard, Trovato, E., Tuci, V., Tueros, Matias, Tusi, E., Ulrich, Ralf, Unger, Michael, Urban, Marcel, Valdes Galicia, J. F., Valino, Ines, Valore, Laura, Den Berg, Ad M., Vazquez, J. R., Vazquez, Ricardo A., Veberic, Darko, Velarde, Alfonso, Venters, Tonia M., Verzi, Valerio, Videla, M., Villasenor Cendejas, Luis Manuel, Vitali, G., Vorobiov, Serguei, Wahlberg, Hernan Pablo, Wahrlich, Philip, Wainberg, O., Warner, Brian D., Westerhoff, Stefan, Whelan, B. J., Wild, N., Wiebusch, Christopher H., Wieczorek, G., Wiencke, Lawrence R., Wilczynska, Barbara, Wilczynski, Henryk, Wileman, Christopher, Winnick, M. G., Worner, G., Wu, H., Wundheiler, B., Younk, Patrick, Yuan, Guofeng, Yushkov, Alexey V., Zas, Enrique, Zavrtanik, Danilo, Zavrtanik, Marko, Zaw, Ingyin, Ziolkowski, M., APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - 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THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), PIERRE AUGER, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut für theoretische Physik, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, and Research unit Astroparticle Physics

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], FOS: Physical sciences, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics (astro-ph.IM), [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract

Technical reports on operations and features of the Pierre Auger Observatory, including ongoing and planned enhancements and the status of the future northern hemisphere portion of the Observatory. Contributions to the 31st International Cosmic Ray Conference, Lodz, Poland, July 2009., Comment: Contributions to the 31st ICRC, Lodz, Poland, July 2009

17. Sensitivity of Extensive Air Showers to Features of Hadronic Interactions at Ultra-High Energies

Author

Ulrich, Ralf, Engel, Ralph, Muller, Steffen, Tanguy Pierog, Schussler, Fabian, and Unger, Michael

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract

We study the dependence of extensive air shower development on the first hadronic interactions at ultra-high energies occurring in the startup phase of the air shower cascade. The interpretation of standard air shower observables depends on the characteristics of these interactions. Thus, it is currently difficult to draw firm conclusions for example on the primary cosmic ray mass composition from the analysis of air shower data. On the other hand, a known primary mass composition would allow us to study hadronic interactions at center of mass energies well above the range that is accessible to accelerators measurements., Submitted to the 31th ICRC, Lodz, Poland, 2009

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