{
  "_oai": {
    "updated": "2021-05-27T00:33:47Z", 
    "id": "oai:repo.scoap3.org:59941", 
    "sets": [
      "JHEP"
    ]
  }, 
  "authors": [
    {
      "affiliations": [
        {
          "country": "Sweden", 
          "value": "Department of Physics and Astronomy, Uppsala University, Box 516, Uppsala, 75108, Sweden", 
          "organization": "Uppsala University"
        }, 
        {
          "country": "Germany", 
          "value": "Institut f\u00fcr Physik und IRIS Adlershof, Humboldt-Universit\u00e4t zu Berlin, Zum Gro\u00dfen Windkanal 6, Berlin, D-12489, Germany", 
          "organization": "Humboldt-Universit\u00e4t zu Berlin"
        }, 
        {
          "country": "Germany", 
          "value": "Max-Planck-Institut f\u00fcr Gravitationsphysik (Albert-Einstein-Institut), M\u00fchlenberg 1, Potsdam, D-14476, Germany", 
          "organization": "Max-Planck-Institut f\u00fcr Gravitationsphysik (Albert-Einstein-Institut)"
        }
      ], 
      "surname": "Mogull", 
      "email": "gustav.mogull@aei.mpg.de", 
      "full_name": "Mogull, Gustav", 
      "given_names": "Gustav"
    }, 
    {
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Institut f\u00fcr Physik und IRIS Adlershof, Humboldt-Universit\u00e4t zu Berlin, Zum Gro\u00dfen Windkanal 6, Berlin, D-12489, Germany", 
          "organization": "Humboldt-Universit\u00e4t zu Berlin"
        }
      ], 
      "surname": "Plefka", 
      "email": "jan.plefka@hu-berlin.de", 
      "full_name": "Plefka, Jan", 
      "given_names": "Jan"
    }, 
    {
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Max-Planck-Institut f\u00fcr Gravitationsphysik (Albert-Einstein-Institut), M\u00fchlenberg 1, Potsdam, D-14476, Germany", 
          "organization": "Max-Planck-Institut f\u00fcr Gravitationsphysik (Albert-Einstein-Institut)"
        }
      ], 
      "surname": "Steinhoff", 
      "email": "jan.steinhoff@aei.mpg.de", 
      "full_name": "Steinhoff, Jan", 
      "given_names": "Jan"
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Classical black hole scattering from a worldline quantum field theory"
    }
  ], 
  "dois": [
    {
      "value": "10.1007/JHEP02(2021)048"
    }
  ], 
  "publication_info": [
    {
      "page_end": "43", 
      "journal_title": "Journal of High Energy Physics", 
      "material": "article", 
      "journal_volume": "2021", 
      "artid": "JHEP02(2021)048", 
      "year": 2021, 
      "page_start": "1", 
      "journal_issue": "2"
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
  "acquisition_source": {
    "date": "2021-05-27T00:30:41.800637", 
    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "abbf0a02be8211eb92440a580a640a05"
  }, 
  "page_nr": [
    43
  ], 
  "license": [
    {
      "url": "https://creativecommons.org/licenses//by/4.0", 
      "license": "CC-BY-4.0"
    }
  ], 
  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2021"
    }
  ], 
  "control_number": "59941", 
  "record_creation_date": "2021-02-05T22:30:22.029744", 
  "_files": [
    {
      "checksum": "md5:34e15142a48b88916258ec2e017b8336", 
      "filetype": "xml", 
      "bucket": "f19d0133-5b09-47fa-aea2-810b293163f9", 
      "version_id": "e38ea8bc-8fc8-4320-9674-0349fa2db4da", 
      "key": "10.1007/JHEP02(2021)048.xml", 
      "size": 14789
    }, 
    {
      "checksum": "md5:1211f822d2ffb13a9b5b0a982db29053", 
      "filetype": "pdf/a", 
      "bucket": "f19d0133-5b09-47fa-aea2-810b293163f9", 
      "version_id": "9da7c5f6-2485-4509-abe7-b0d098d8a895", 
      "key": "10.1007/JHEP02(2021)048_a.pdf", 
      "size": 816492
    }
  ], 
  "collections": [
    {
      "primary": "Journal of High Energy Physics"
    }
  ], 
  "arxiv_eprints": [
    {
      "categories": [
        "hep-th", 
        "gr-qc"
      ], 
      "value": "2010.02865"
    }
  ], 
  "abstracts": [
    {
      "source": "Springer", 
      "value": "A precise link is derived between scalar-graviton S-matrix elements and expectation values of operators in a worldline quantum field theory (WQFT), both used to describe classical scattering of black holes. The link is formally provided by a worldline path integral representation of the graviton-dressed scalar propagator, which may be inserted into a traditional definition of the S-matrix in terms of time-ordered correlators. To calculate expectation values in the WQFT a new set of Feynman rules is introduced which treats the gravitational field h  \u03bc\u03bd (x) and position   <math> <msubsup> <mi>x</mi> <mi>i</mi> <mi>\u03bc</mi> </msubsup> <mfenced> <msub> <mi>\u03c4</mi> <mi>i</mi> </msub> </mfenced> </math>  $$ {x}_i^{\\mu}\\left({\\tau}_i\\right) $$  of each black hole on equal footing. Using these both the 3PM three-body gravitational radiation \u2329h  \u03bcv (k)\u232a and 2PM two-body deflection   <math> <mi>\u0394</mi> <msubsup> <mi>p</mi> <mi>i</mi> <mi>\u03bc</mi> </msubsup> </math>  $$ \\Delta {p}_i^{\\mu } $$  from classical black hole scattering events are obtained. The latter can also be obtained from the eikonal phase of a 2 \u2192 2 scalar S-matrix, which we show corresponds to the free energy of the WQFT."
    }
  ], 
  "imprints": [
    {
      "date": "2021-02-05", 
      "publisher": "Springer"
    }
  ]
}