{"as_of":"2026-08-16T23:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fc434f9c278a51ca0c78be99f73b8355d9668eab124c9cce8dbc6a09d426728b","coverage":[{"denominator":28,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":28,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T10:27:35.109989Z","state":"measured"},{"denominator":28,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":28,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/1908.11265/citation-record","integrity":"/paper/1908.11265/integrity","json":"/paper/1908.11265/citation-record.json","paper":"/paper/1908.11265"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.751780Z","title":"Taylor expansion of the solution (64) is u(x) =−e0 [ 1 +b2 0(x−x0)2 + b4 0 3 (x−x0)4 +","venue":null,"work_id":"26a9e594-99ad-490b-af6e-1174593e739e","year":null},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:34.978991Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:769df8d60ba4239b6af9ed27c37eb6a531b043a243a0a1e81464cb55ac86180f","observation_id":"d9ed2dc3-72d2-4849-aa35-54c8c2f4317f","resolution":{"observed_at":"2026-08-14T10:27:35.756385Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.720851Z","title":"Kazanas, Astrophys","venue":null,"work_id":"53bab0b3-b723-41ff-a83d-3696d0b8416b","year":1980},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:34.994336Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:51bd7427007b15ca7bc1f3a68b1cd5e8d4f4e34bd18e2abe64ad696d0ec36ccb","observation_id":"8841a287-6c53-4a2c-8c84-6ffd7b60db3a","resolution":{"observed_at":"2026-08-14T10:27:35.725868Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/0307335","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.291417Z","title":"Masi et al","venue":null,"work_id":"b39a0031-9cfa-4fb7-8b27-ca6855364246","year":2002},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:34.989717Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:d8107ac351bc948a2b98512f02d5e41809a0f9909b7d349d9199ffb82717ec5f","observation_id":"434eeb1f-480b-4c2c-97c4-cff39219b9e9","resolution":{"observed_at":"2026-08-14T10:27:35.299693Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.694852Z","title":"Padmanabhan, Curr","venue":null,"work_id":"8bdd3aa0-237c-4e24-8dd6-88eec5be8596","year":2005},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.004800Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:2d533b5aeb04a02a2f4c6844724a6366ecf9227bdc15774eefc55d7e494c3250","observation_id":"ee91e1c5-718e-4ce6-a0a4-54d414a7187f","resolution":{"observed_at":"2026-08-14T10:27:35.700482Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:34.999013Z","title":"Nojiri and S","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:34.999013Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:48ecb43ffb093a3ac891136d01f38a1e53b20eacb3fc4a5860a1b69504e13997","observation_id":"ca05dab8-5dca-407e-ad30-1c1563b842b6","resolution":{"observed_at":"2026-08-14T10:27:34.999013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.662874Z","title":null,"venue":null,"work_id":"82fb9968-4c32-4545-b9b3-42d92737c0c9","year":1968},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.015512Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:ff202267bdbb7d581c9e853a78c5a0f76e8405f8a2336effcb6d278154f50a84","observation_id":"06590675-1ed7-429e-bbac-7e785942c468","resolution":{"observed_at":"2026-08-14T10:27:35.667958Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.679083Z","title":null,"venue":null,"work_id":"57a767ea-9a2f-47c2-8f28-53eb91aff1fb","year":null},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.009962Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:c3c853d7c227f5acaa01db3e05793b2eaa0829ae3b2c945b96ccdc70057fb1fb","observation_id":"e71feac5-031c-4861-a699-9a0387215f35","resolution":{"observed_at":"2026-08-14T10:27:35.684114Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.631120Z","title":"Pinney, Proc","venue":null,"work_id":"ab50cb1f-29c0-4f72-9859-fe9045c3721d","year":1950},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.025915Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:166b5681295f000c6d5201918ecf4bd458292d3a3faddcd24befab3496fcb62b","observation_id":"c5e605bf-08bb-4ea6-a999-b107f29549fa","resolution":{"observed_at":"2026-08-14T10:27:35.635781Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.647210Z","title":null,"venue":null,"work_id":"cf6919ff-6c2f-462b-8018-63f8c8648d7f","year":2002},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.020852Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:d181fff16a97bbbf625901188c6b044f6daf1721c5e986757d4a7896d61fb67d","observation_id":"3cfa6c3e-fec1-4e65-a529-23902f0b203f","resolution":{"observed_at":"2026-08-14T10:27:35.652078Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.599992Z","title":"Lutzky, Phys","venue":null,"work_id":"ac567389-1732-4d5e-91de-d715f1203e09","year":1978},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.035465Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:e31d9b29b5c5f0e2858d94e3362edea3d42043350bdee2777a0fa7b74864cfb2","observation_id":"bee5812f-8add-4923-a66c-884da92a25c4","resolution":{"observed_at":"2026-08-14T10:27:35.604945Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.615834Z","title":null,"venue":null,"work_id":"c6242c3b-9be2-4c9f-801b-68f596bed861","year":1930},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.030469Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:70fdb7a819df623b52ed06f30cdeb600681d4156366ba998baeb8e6d2aacc44f","observation_id":"311a3128-88f3-423d-a4fb-08a08488dddb","resolution":{"observed_at":"2026-08-14T10:27:35.620466Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0302120","last_updated":"2003-02-28T12:55:31Z","snapshot_observed_at":"2026-08-09T10:59:12.505192Z","submitted_at":"2003-02-28T12:55:31Z","title":"On 3+1 Dimensional Friedman-Robertson-Walker Universes with Matter","version":1},"cited_work":{"arxiv_id":"gr-qc/0302120","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0302120","snapshot_observed_at":"2026-08-14T10:27:35.212766Z","title":"On 3+1 Dimensional Friedman-Robertson-Walker Universes with Matter","venue":"gr-qc","work_id":"a81ac0f9-da32-4b64-9850-e06bc7f01023","year":2003},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.045102Z"},"links":{"cited_paper":"/paper/gr-qc/0302120","citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:44bc26cb111c607b08713c84110203aa412a707780178741baffe85637a4a34b","observation_id":"731c3c44-74ce-4189-9532-c3832bcade8d","resolution":{"observed_at":"2026-08-14T10:27:35.218248Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.584970Z","title":null,"venue":null,"work_id":"5d498f7a-f6fd-4ced-8a39-49a609e0cacd","year":2003},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.040035Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:99399c30a86737775396cfd1c99f808079d259f51e43f511663b25371f86e13a","observation_id":"0f24413f-f0a2-43d6-be1d-c40d2151149a","resolution":{"observed_at":"2026-08-14T10:27:35.589862Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.553498Z","title":"D’Ambroise, Int","venue":null,"work_id":"f84fba94-650f-4a93-ba78-9fea13176c67","year":2008},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.054539Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:d2c38ce16b12d6247c721786001cb3e6bbd3c2830be3fe74e6a2eddccb10a591","observation_id":"c0481622-806b-4d17-8014-48b8d605a7ee","resolution":{"observed_at":"2026-08-14T10:27:35.558935Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.569400Z","title":null,"venue":null,"work_id":"9f4a397b-161d-4eb1-93df-56d2aeebf3c8","year":2006},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.050177Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:c3c9e116c456b30a8258738979bd7dc75ddfaec362df40f7f72927b356c1c6dc","observation_id":"731ce96d-79e2-456e-adbb-4abefa17bfe5","resolution":{"observed_at":"2026-08-14T10:27:35.573882Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.425272Z","title":"Kamenshchik and G","venue":null,"work_id":"d354ece6-32aa-493e-873b-13c1b38629be","year":2009},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.064289Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:5b8b4ed1c65fe046ea9a0af8596a612d888b483cf64eb49560bdf157f017dfb8","observation_id":"0ba9ac83-86c3-45ae-b5cf-3213dca9ee28","resolution":{"observed_at":"2026-08-14T10:27:35.431120Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.538167Z","title":null,"venue":null,"work_id":"d227c3c3-0c07-44d9-9ec1-041ca6baec1b","year":2004},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.059591Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:2c2b8346ce8fe11c9630c981498bac4c9d58fcf54065659ae4999b7baa35f5ec","observation_id":"66f6dbc5-8add-4e94-87a2-f3a1c0049f8c","resolution":{"observed_at":"2026-08-14T10:27:35.543072Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.393477Z","title":"D’Ambroise and F","venue":null,"work_id":"cff51016-81a7-41c7-805d-822b3c53e945","year":2007},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.073128Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:1ad476e7cc271106c03c9253758c62b198551a3ddfc2bb7c1f469f0f328858c3","observation_id":"728e0e05-ac7d-45f0-825a-ebb4196f9d2e","resolution":{"observed_at":"2026-08-14T10:27:35.398611Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.409509Z","title":null,"venue":null,"work_id":"62be8e44-c269-405b-aea5-768a82523826","year":2005},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.068903Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:ede6d39f35b3153c07eb648fa67a376a436c09fa3ee322076a71bd68efc793db","observation_id":"ab0be081-fa46-4aad-8f6b-194717e5b0eb","resolution":{"observed_at":"2026-08-14T10:27:35.414535Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.360660Z","title":"D’Ambroise and F","venue":null,"work_id":"3369ca29-15dd-49e8-a80b-02d07cd27fdc","year":2011},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.081712Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:6cae1d6581f1053c1e2f0846956d77c1de5456be46e370ed153a84502f1eb0b1","observation_id":"5e5ef44f-6928-4237-86ed-5cf6546ee9d3","resolution":{"observed_at":"2026-08-14T10:27:35.365767Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.376823Z","title":"Gumjudpai, Gen","venue":null,"work_id":"ee8c6b92-053d-4ac3-baec-03e7c5b9081f","year":2009},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.077314Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:6c4baf8b8ad42fadd581222a3c5c66aa667877a2d0f9d7648f41226ab5b3e889","observation_id":"b4a35b53-5dad-4cb8-8f60-366b9f619a10","resolution":{"observed_at":"2026-08-14T10:27:35.381844Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.736089Z","title":"Hence it can not be probabilistically interpreted","venue":null,"work_id":"277a888c-36bc-4f6e-8baa-2595d9aea58e","year":null},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:34.985183Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:b2b9596c055a8cd6ca971d03132b2ac926c5e27ea50c1997ad1e17c14df5f766","observation_id":"d9b27dc9-6a27-48dd-9282-3425c9524b43","resolution":{"observed_at":"2026-08-14T10:27:35.741470Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1309.7181","last_updated":"2013-09-27T09:44:38Z","snapshot_observed_at":"2026-08-15T00:01:34.513363Z","submitted_at":"2013-09-27T09:44:38Z","title":"Scalar Field Cosmologies Hidden Within the Nonlinear Schrodinger Equation","version":1},"cited_work":{"arxiv_id":"1309.7181","doi":null,"metadata_source":"pith","pith_arxiv_id":"1309.7181","snapshot_observed_at":"2026-08-14T10:27:35.189661Z","title":"Scalar Field Cosmologies Hidden Within the Nonlinear Schrodinger Equation","venue":"gr-qc","work_id":"bfdc1643-471a-4f19-9ab5-ff597cddd743","year":2013},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.086800Z"},"links":{"cited_paper":"/paper/1309.7181","citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:ab639b2e8f06d01b094b4f0a855e1fefa14314de216f7526251900f9cc57960d","observation_id":"3378a124-05f6-4529-89e4-8e4f8ffa108d","resolution":{"observed_at":"2026-08-14T10:27:35.196014Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.345018Z","title":"Gumjudpai, Astropart","venue":null,"work_id":"e7f6229e-bbf5-40e6-a96e-6661073d4bfa","year":2008},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.091560Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:ba3348e2f6b2ec519be80c97ee94fe921e658c9364bcc1f02e4a7ce04b43e6c8","observation_id":"79a4cb72-0cd1-4999-aefb-6adb534d8d2f","resolution":{"observed_at":"2026-08-14T10:27:35.350220Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.329474Z","title":"Phetnora, R","venue":null,"work_id":"3c21ca06-5da4-4561-8a09-53a3a8bec04b","year":2010},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.096155Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:2fbd00a5625b648cd3b9d7ee9bea0a27df270996022f966254781f6d881ec6e8","observation_id":"bcba6148-9f47-479f-8965-6a700ed4ff92","resolution":{"observed_at":"2026-08-14T10:27:35.334447Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0904.2746","last_updated":"2009-04-17T17:04:41Z","snapshot_observed_at":"2026-08-15T05:50:19.392736Z","submitted_at":"2009-04-17T17:04:41Z","title":"Scalar field cosmology: its non-linear Schr\\\"{o}dinger-type formulation","version":1},"cited_work":{"arxiv_id":"0904.2746","doi":null,"metadata_source":"pith","pith_arxiv_id":"0904.2746","snapshot_observed_at":"2026-08-14T10:27:35.169576Z","title":"Scalar field cosmology: its non-linear Schr\\\"{o}dinger-type formulation","venue":"gr-qc","work_id":"aad1f3e9-6882-45c2-b00c-d12794659d9d","year":2009},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.100464Z"},"links":{"cited_paper":"/paper/0904.2746","citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:6882d9a02ac3e772408a364cd1de2fcbf85f3ea0ac015c4668c3729ff64ff6c1","observation_id":"222f5d7f-2711-4d18-9801-109c8c50fc36","resolution":{"observed_at":"2026-08-14T10:27:35.174459Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T10:27:35.312247Z","title":"Gumjudpai, JCAP 0809, 028 (2008)","venue":null,"work_id":"de39e8d0-19f2-438f-a423-05d661391546","year":2008},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.105608Z"},"links":{"citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:01074c070c0b19ac85d448f757f113240130365a1d92ff7e76f1cf9157a51cb5","observation_id":"60b592a5-7ab5-476f-aa1a-0b6ad6507fbc","resolution":{"observed_at":"2026-08-14T10:27:35.317989Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1005.1410","last_updated":"2010-05-09T17:11:14Z","snapshot_observed_at":"2026-08-15T05:19:33.530453Z","submitted_at":"2010-05-09T17:11:14Z","title":"Generalized EMP and nonlinear Schrodinger-type reformulations of some scalar field cosmological models","version":1},"cited_work":{"arxiv_id":"1005.1410","doi":null,"metadata_source":"pith","pith_arxiv_id":"1005.1410","snapshot_observed_at":"2026-08-14T10:27:35.145979Z","title":"Generalized EMP and nonlinear Schrodinger-type reformulations of some scalar field cosmological models","venue":"gr-qc","work_id":"c7148271-45f4-4f51-9a37-be3a515a7292","year":2010},"citing_paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T10:27:35.109989Z"},"links":{"cited_paper":"/paper/1005.1410","citing_paper":"/paper/1908.11265"},"observation_digest":"sha256:a2c0fbf4ce6ebaba0d82214c03e9738bbcec04a79f660136e03e3b9eb53455ac","observation_id":"08510996-ab92-46d8-b60c-e21ff6988399","resolution":{"observed_at":"2026-08-14T10:27:35.152963Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.11265","last_updated":"2020-03-10T18:00:25Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T13:34:54.095898Z","submitted_at":"2019-08-29T14:43:22Z","title":"Non-linear Schr\\\"{o}dinger-type formulation of scalar field cosmology: two barotropic fluids and exact solutions"},"reference_resolution":{"displayed":28,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":9,"verified_exact":4,"verified_fuzzy":14},"total_outbound_references":28},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 28 of 28 outbound references and 0 inbound Pith citation observations for arXiv:1908.11265."}