Properties of Doubly Heavy Baryons

We revisited the mass spectra of the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>c</mi><mi>c</mi></mrow><mrow><mo>+<...

Full description

Bibliographic Details
Main Authors: Zalak Shah, Amee Kakadiya, Keval Gandhi, Ajay Kumar Rai
Format: Article
Language:English
Published: MDPI AG 2021-09-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/7/9/337
id doaj-e747e6fdb25e403d9c7b5087b97f3b47
record_format Article
collection DOAJ
language English
format Article
sources DOAJ
author Zalak Shah
Amee Kakadiya
Keval Gandhi
Ajay Kumar Rai
spellingShingle Zalak Shah
Amee Kakadiya
Keval Gandhi
Ajay Kumar Rai
Properties of Doubly Heavy Baryons
Universe
mass spectra
potential model
radiative transitions
author_facet Zalak Shah
Amee Kakadiya
Keval Gandhi
Ajay Kumar Rai
author_sort Zalak Shah
title Properties of Doubly Heavy Baryons
title_short Properties of Doubly Heavy Baryons
title_full Properties of Doubly Heavy Baryons
title_fullStr Properties of Doubly Heavy Baryons
title_full_unstemmed Properties of Doubly Heavy Baryons
title_sort properties of doubly heavy baryons
publisher MDPI AG
series Universe
issn 2218-1997
publishDate 2021-09-01
description We revisited the mass spectra of the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>c</mi><mi>c</mi></mrow><mrow><mo>+</mo><mo>+</mo></mrow></msubsup></semantics></math></inline-formula> baryon with positive and negative parity states using Hypercentral Constituent Quark Model Scheme with Coloumb plus screened potential. The ground state of the baryon has been determined by the LHCb experiment, and the anticipated excited state masses of the baryon have been compared with several theoretical methodologies. The transition magnetic moments of all heavy baryons <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>c</mi><mi>c</mi></mrow><mrow><mo>+</mo><mo>+</mo></mrow></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>c</mi><mi>c</mi></mrow><mo>+</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ω</mo><mrow><mi>c</mi><mi>c</mi></mrow><mo>+</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>b</mi></mrow><mn>0</mn></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>b</mi></mrow><mo>−</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ω</mo><mrow><mi>b</mi><mi>b</mi></mrow><mo>−</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>c</mi></mrow><mo>+</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>c</mi></mrow><mn>0</mn></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ω</mo><mrow><mi>b</mi><mi>c</mi></mrow><mn>0</mn></msubsup></semantics></math></inline-formula> are also calculated and their values are −1.013 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 1.048 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.961 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, −1.69 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.73 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.48 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, −1.39 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.94 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula> and 0.710 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, respectively.
topic mass spectra
potential model
radiative transitions
url https://www.mdpi.com/2218-1997/7/9/337
work_keys_str_mv AT zalakshah propertiesofdoublyheavybaryons
AT ameekakadiya propertiesofdoublyheavybaryons
AT kevalgandhi propertiesofdoublyheavybaryons
AT ajaykumarrai propertiesofdoublyheavybaryons
_version_ 1716868733009395712
spelling doaj-e747e6fdb25e403d9c7b5087b97f3b472021-09-26T01:34:47ZengMDPI AGUniverse2218-19972021-09-01733733710.3390/universe7090337Properties of Doubly Heavy BaryonsZalak Shah0Amee Kakadiya1Keval Gandhi2Ajay Kumar Rai3Department of Physics, S.V. National Institute of Technology, Surat 395007, IndiaDepartment of Physics, S.V. National Institute of Technology, Surat 395007, IndiaDepartment of Physics, S.V. National Institute of Technology, Surat 395007, IndiaDepartment of Physics, S.V. National Institute of Technology, Surat 395007, IndiaWe revisited the mass spectra of the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>c</mi><mi>c</mi></mrow><mrow><mo>+</mo><mo>+</mo></mrow></msubsup></semantics></math></inline-formula> baryon with positive and negative parity states using Hypercentral Constituent Quark Model Scheme with Coloumb plus screened potential. The ground state of the baryon has been determined by the LHCb experiment, and the anticipated excited state masses of the baryon have been compared with several theoretical methodologies. The transition magnetic moments of all heavy baryons <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>c</mi><mi>c</mi></mrow><mrow><mo>+</mo><mo>+</mo></mrow></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>c</mi><mi>c</mi></mrow><mo>+</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ω</mo><mrow><mi>c</mi><mi>c</mi></mrow><mo>+</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>b</mi></mrow><mn>0</mn></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>b</mi></mrow><mo>−</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ω</mo><mrow><mi>b</mi><mi>b</mi></mrow><mo>−</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>c</mi></mrow><mo>+</mo></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ξ</mo><mrow><mi>b</mi><mi>c</mi></mrow><mn>0</mn></msubsup></semantics></math></inline-formula>, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msubsup><mo>Ω</mo><mrow><mi>b</mi><mi>c</mi></mrow><mn>0</mn></msubsup></semantics></math></inline-formula> are also calculated and their values are −1.013 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 1.048 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.961 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, −1.69 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.73 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.48 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, −1.39 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, 0.94 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula> and 0.710 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi mathvariant="sans-serif">μ</mi><mi mathvariant="normal">N</mi></msub></semantics></math></inline-formula>, respectively.https://www.mdpi.com/2218-1997/7/9/337mass spectrapotential modelradiative transitions