[
    {
        "id": "authors:hcdze-1c664",
        "collection": "authors",
        "collection_id": "hcdze-1c664",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210504-124646617",
        "type": "book_section",
        "title": "LIGO and Science Diplomacy",
        "book_title": "International Cooperation for Enhancing Nuclear Safety, Security, Safeguards and Non-proliferation",
        "author": [
            {
                "family_name": "Barish",
                "given_name": "Barry",
                "clpid": "Barish-B-C"
            }
        ],
        "contributor": [
            {
                "family_name": "Maiani",
                "given_name": "Luciano",
                "clpid": "Maiani-Luciano"
            },
            {
                "family_name": "Jeanloz",
                "given_name": "Raymond",
                "clpid": "Jeanloz-Raymond"
            },
            {
                "family_name": "Lowenthal",
                "given_name": "Micah",
                "clpid": "Lowenthal-Micah"
            },
            {
                "family_name": "Plastino",
                "given_name": "Wolfango",
                "clpid": "Plastino-Wolfango"
            }
        ],
        "abstract": "The discovery of gravitational waves in LIGO captured the imagination of the public, worldwide. Why? The answer is one that is fundamental to the human race. A universal feature that sets humans apart from other living species is our curiosity about nature and the world we live in. Some of this knowledge is self-serving, like how to cope with diseases or how to improve our way of life. However, our curiosity goes well beyond just satisfying needs, as it includes our fascination with the stars, the origin of the universe, or just simply our understanding how things work.",
        "doi": "10.1007/978-3-030-42913-3_27",
        "isbn": "978-3-030-42912-6",
        "publisher": "Springer",
        "place_of_publication": "Cham",
        "publication_date": "2020-04-08",
        "pages": "193-198"
    },
    {
        "id": "authors:rzkfx-e7074",
        "collection": "authors",
        "collection_id": "rzkfx-e7074",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160420-075353860",
        "type": "book_section",
        "title": "Science of Extreme Light Infrastructure",
        "book_title": "1st International Conference on Light at Extreme Intensities (LEI 2009)",
        "author": [
            {
                "family_name": "Tajima",
                "given_name": "Toshiki",
                "clpid": "Tajima-Toshiki"
            },
            {
                "family_name": "Barish",
                "given_name": "Barry C.",
                "clpid": "Barish-B-C"
            },
            {
                "family_name": "Barty",
                "given_name": "C. P.",
                "clpid": "Barty-C-P"
            },
            {
                "family_name": "Bulanov",
                "given_name": "Sergei",
                "clpid": "Bulanov-S"
            },
            {
                "family_name": "Chen",
                "given_name": "Pisin",
                "clpid": "Chen-Pisin"
            },
            {
                "family_name": "Feldhaus",
                "given_name": "Josef",
                "clpid": "Feldhaus-J"
            },
            {
                "family_name": "Hajdu",
                "given_name": "Janos",
                "clpid": "Hajdu-J"
            },
            {
                "family_name": "Keitel",
                "given_name": "Christoph H.",
                "clpid": "Keitel-C-H"
            },
            {
                "family_name": "Kieffer",
                "given_name": "Jean-Claude",
                "clpid": "Kieffer-J-C"
            },
            {
                "family_name": "Ko",
                "given_name": "Do-Kyeong",
                "clpid": "Ko-Do-Kyeong"
            },
            {
                "family_name": "Leemans",
                "given_name": "Wim",
                "clpid": "Leemans-W"
            },
            {
                "family_name": "Normand",
                "given_name": "Didier",
                "clpid": "Normand-D"
            },
            {
                "family_name": "Palumbo",
                "given_name": "Luigi",
                "clpid": "Palumbo-L"
            },
            {
                "family_name": "Rzazewski",
                "given_name": "Kazimierz",
                "clpid": "Rzazewski-K"
            },
            {
                "family_name": "Sergeev",
                "given_name": "Alexander",
                "clpid": "Sergeev-A"
            },
            {
                "family_name": "Sheng",
                "given_name": "Zheng-Ming",
                "clpid": "Sheng-Zheng-Ming"
            },
            {
                "family_name": "Takasaki",
                "given_name": "Fumihiko",
                "clpid": "Takasaki-Fumihiko"
            },
            {
                "family_name": "Teshima",
                "given_name": "Masahiro",
                "clpid": "Teshima-Masahiro"
            }
        ],
        "contributor": [
            {
                "family_name": "Dumitras",
                "given_name": "Dan",
                "clpid": "Dumitras-D"
            }
        ],
        "abstract": "The infrastructure of Extreme Light Infrastructure (ELI) provides an unprecedented opportunity for a broad range of frontier science. Its highest ever intensity of lasers, as well as high fluence, high power, and/or ultrafast optical characteristics carve out new territories of discovery, ranging from attosecond science to photonuclear science, laser acceleration and associated beams, and high field science (Four Pillars of ELI). Its applications span from medicine, biology, engineering, energy, chemistry, physics, and fundamental understanding of the Universe. The relativistic optics that intense lasers have begun exploring may be extended into a new regime of ultra\u2010relativistic regime, where even protons fly relativistically in the optical fields. ELI provides the highest intensity to date such that photon fields begin to feel even the texture of vacuum. This is a singular appeal of ELI with its relatively modest infrastructure (compared to the contemporary largest scientific infrastructures), yet provides an exceptional avenue along which the 21st Century science and society need to answer the toughest questions. The intensity frontier simultaneously brings in the energy horizon (TeV and PeV) as well as temporal frontier (attoseconds and zeptoseconds). It also turns over optics of atoms and molecules into that of nuclei with the ability to produce monoenergetic collimated \u03b3\u2010ray photons. As such, the ELI concept acutely demands an effort to encompass and integrate its Four Pillars.",
        "doi": "10.1063/1.3426041",
        "isbn": "978-0-7354-0771-8",
        "publisher": "American Institute of Physics",
        "place_of_publication": "Melville, NY",
        "publication_date": "2010-04-16",
        "pages": "11-35"
    },
    {
        "id": "authors:stvb9-b8j75",
        "collection": "authors",
        "collection_id": "stvb9-b8j75",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20111003-143522581",
        "type": "book_section",
        "title": "First generation interferometers",
        "book_title": "Astrophysical sources for ground-based gravitational wave detectors",
        "author": [
            {
                "family_name": "Barish",
                "given_name": "Barry C.",
                "clpid": "Barish-B-C"
            }
        ],
        "contributor": [
            {
                "family_name": "Centrella",
                "given_name": "Joan M.",
                "clpid": "Centrella-J-M"
            }
        ],
        "abstract": "The status and plans for the first generation long baseline suspended mass interferometers TAMA, GEO, LIGO and Virgo are presented, as well as the expected performances.",
        "doi": "10.1063/1.1387295",
        "isbn": "0-7354-0014-8",
        "publisher": "American Institute of Physics",
        "place_of_publication": "Melville, Ny",
        "publication_date": "2001-06-22",
        "pages": "3-14"
    },
    {
        "id": "authors:p76jt-yye61",
        "collection": "authors",
        "collection_id": "p76jt-yye61",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200212-152223047",
        "type": "book_section",
        "title": "Gravitational Waves",
        "book_title": "Cosmic Radiations: From Astronomy to Particle Physics",
        "author": [
            {
                "family_name": "Barish",
                "given_name": "Barry C.",
                "clpid": "Barish-B-C"
            }
        ],
        "contributor": [
            {
                "family_name": "Giacomelli",
                "given_name": "Giorgio",
                "clpid": "Giacomelli-G"
            },
            {
                "family_name": "Spurio",
                "given_name": "Maurizio",
                "clpid": "Spurio-M"
            },
            {
                "family_name": "Derkaoui",
                "given_name": "Jamal Eddine",
                "clpid": "Derkaoui-J-E"
            }
        ],
        "abstract": "The effort to develop suspended mass interferometers for gravitational wave detection has lead to an ambitious new set of long baseline interferometers that will soon become operational. These detectors are based on the effect of a propagating gravitational wave to deform space in a quadrupolar form. The characteristics of the deformation are indicated in figure 1.",
        "doi": "10.1007/978-94-010-0634-7_3",
        "isbn": "978-1-4020-0120-8",
        "publisher": "Springer",
        "place_of_publication": "Dordrecht",
        "publication_date": "2001",
        "pages": "47-65"
    },
    {
        "id": "authors:8mh59-zjv03",
        "collection": "authors",
        "collection_id": "8mh59-zjv03",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20111123-071400948",
        "type": "book_section",
        "title": "Amaldi Meeting Introduction",
        "book_title": "Gravitational Waves",
        "author": [
            {
                "family_name": "Barish",
                "given_name": "Barry C.",
                "clpid": "Barish-B-C"
            }
        ],
        "contributor": [
            {
                "family_name": "Amaldi",
                "given_name": "E.",
                "clpid": "Amaldi-E"
            },
            {
                "family_name": "Meshkov",
                "given_name": "S.",
                "clpid": "Meshkov-S"
            }
        ],
        "abstract": "Welcome to Caltech and the 3rd Edoardo Amaldi Conference on Gravitational Waves.\nObviously, something must be very interesting to bring more than 250 scientists from\naround the world to Pasadena in July for this particular meeting. In fact, July in\nSouthern California does have many attractions, in addition to the good weather and\ncool nights. For this conference, we have arranged a visit to the new Getty Museum on\nour excursion day. This is meant to make your stay more pleasant, but is not the real\nreason we have gathered here. This meeting addresses the detection of gravitational\nwaves, a much-anticipated event.",
        "doi": "10.1063/1.1291835",
        "isbn": "9781563969447",
        "publisher": "American Institute of Physics",
        "place_of_publication": "Melville, N.Y.",
        "publication_date": "2000-06-15",
        "pages": "3-4"
    },
    {
        "id": "authors:h7rbd-tad59",
        "collection": "authors",
        "collection_id": "h7rbd-tad59",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180830-102156608",
        "type": "book_section",
        "title": "Investigations of High Energy Neutrino Interactions in the Caltech-Fermilab Experiment",
        "book_title": "Weak and Electromagnetic Interactions at High Energies: Carg\u00e8se 1975",
        "author": [
            {
                "family_name": "Barish",
                "given_name": "B. C.",
                "clpid": "Barish-B-C"
            }
        ],
        "contributor": [
            {
                "family_name": "L\u00e9vy",
                "given_name": "Maurice",
                "clpid": "L\u00e9vy-M"
            },
            {
                "family_name": "Basdevant",
                "given_name": "Jean-Louis",
                "clpid": "Basdevant-J-L"
            },
            {
                "family_name": "Speiser",
                "given_name": "David",
                "clpid": "Speiser-D"
            },
            {
                "family_name": "Gastmans",
                "given_name": "Raymond",
                "clpid": "Gastmans-R"
            }
        ],
        "abstract": "Recent results from the Caltech-Fermilab experiment are presented. This includes information on the neutral current coupling, charged current differential distributions, and the observation of events with two muons in the final state. \n\nThe prime focus of our group this past year has been to follow up the discovery of neutral currents with a set of measurements especially designed to determined more about the nature of the neutral current interaction. The first experiment of this type was performed in october\u2013november 1974 and I will report here preliminary conclusions from that data. \n\nAs an exciting side product of this neutral current experiment we have observed neutrino events with two muons in the final state. These events appear to be due to new and as yet unexplained physics! I will describe the observation of these events, their characteristics, and comment on possible physics explanations. \n\nWe have also studied our ordinary charged current events (\u03c5 + N \u2192 \u03bc + hadrons), especially with antineutrinos, looking for any possible thresholds or anomalies. I will also describe our present understanding and interpretation of this charged current process.",
        "doi": "10.1007/978-1-4684-0862-1_4",
        "isbn": "978-1-4684-0864-5",
        "publisher": "Springer",
        "place_of_publication": "Boston, MA",
        "publication_date": "1976",
        "pages": "195-224"
    }
]