The paper deals with Warm Inflationary scenario in FLRW with torsion both from theoretical and observational point of view. In the background of flat FLRW model the Hubble parameter is found to be proportional to the torsion function and warm inflation is examined both in weak and strong dissipation regimes for the power law choice of potential using slow-roll approximation with quasi-stable criteria for radiation. The slow-roll parameters, no.of e-folds, scalar spectral index, and tensor-to-scalar ratio are determined in the present model for mainly three choices of the dissipation coefficient $$\Gamma $$ using the Planck data set. Finally, we focus on single-field chaotic quartic potential with the above choices of the dissipation coefficient to confront the warm inflation observational predictions directly with the latest observational data set.
{ "_oai": { "updated": "2023-10-25T18:31:08Z", "id": "oai:repo.scoap3.org:80505", "sets": [ "EPJC" ] }, "authors": [ { "affiliations": [ { "country": "India", "value": "Department of Mathematics, Jadavpur University, Kolkata, 700032, India", "organization": "Jadavpur University" } ], "surname": "Chakraborty", "email": "chakmadhu1997@gmail.com", "full_name": "Chakraborty, Madhukrishna", "given_names": "Madhukrishna" }, { "affiliations": [ { "country": "India", "value": "Department of Mathematics, Jadavpur University, Kolkata, 700032, India", "organization": "Jadavpur University" } ], "surname": "Sardar", "email": "gopalsardar.87@gmail.com", "full_name": "Sardar, Gopal", "given_names": "Gopal" }, { "affiliations": [ { "country": "India", "value": "Department of Mathematics, Jadavpur University, Kolkata, 700032, India", "organization": "Jadavpur University" } ], "surname": "Bose", "email": "bose.akash13@gmail.com", "full_name": "Bose, Akash", "given_names": "Akash" }, { "affiliations": [ { "country": "India", "value": "Department of Mathematics, Jadavpur University, Kolkata, 700032, India", "organization": "Jadavpur University" } ], "surname": "Chakraborty", "email": "schakraborty.math@gmail.com", "full_name": "Chakraborty, Subenoy", "given_names": "Subenoy" } ], "titles": [ { "source": "Springer", "title": "Theoretical and observational prescription of warm-inflation in FLRW universe with torsion" } ], "dois": [ { "value": "10.1140/epjc/s10052-023-12030-8" } ], "publication_info": [ { "page_end": "14", "journal_title": "European Physical Journal C", "material": "article", "journal_volume": "83", "artid": "s10052-023-12030-8", "year": 2023, "page_start": "1", "journal_issue": "9" } ], "$schema": "http://repo.scoap3.org/schemas/hep.json", "acquisition_source": { "date": "2023-10-25T18:30:43.378321", "source": "Springer", "method": "Springer", "submission_number": "816eff8e736411eea066664922b6a1d4" }, "page_nr": [ 14 ], "license": [ { "url": "https://creativecommons.org/licenses//by/4.0", "license": "CC-BY-4.0" } ], "copyright": [ { "holder": "The Author(s)", "year": "2023" } ], "control_number": "80505", "record_creation_date": "2023-09-26T12:30:26.081051", "_files": [ { "checksum": "md5:186602e2e553b66005c9a5ef2289cf6f", "filetype": "xml", "bucket": "14b66af9-f948-4009-ad62-8d65c9b1f302", "version_id": "ba74ea98-3ef1-4741-a2c2-416f485cac27", "key": "10.1140/epjc/s10052-023-12030-8.xml", "size": 12291 }, { "checksum": "md5:465c6af007a430f88d52ece8bfffb2fb", "filetype": "pdf/a", "bucket": "14b66af9-f948-4009-ad62-8d65c9b1f302", "version_id": "170df570-df2e-4c8a-a133-dbe3fd147583", "key": "10.1140/epjc/s10052-023-12030-8_a.pdf", "size": 1149897 } ], "collections": [ { "primary": "European Physical Journal C" } ], "abstracts": [ { "source": "Springer", "value": "The paper deals with Warm Inflationary scenario in FLRW with torsion both from theoretical and observational point of view. In the background of flat FLRW model the Hubble parameter is found to be proportional to the torsion function and warm inflation is examined both in weak and strong dissipation regimes for the power law choice of potential using slow-roll approximation with quasi-stable criteria for radiation. The slow-roll parameters, no.of e-folds, scalar spectral index, and tensor-to-scalar ratio are determined in the present model for mainly three choices of the dissipation coefficient $$\\Gamma $$ <math> <mi>\u0393</mi> </math> using the Planck data set. Finally, we focus on single-field chaotic quartic potential with the above choices of the dissipation coefficient to confront the warm inflation observational predictions directly with the latest observational data set." } ], "imprints": [ { "date": "2023-09-26", "publisher": "Springer" } ] }