Deeply bound dibaryon is incompatible with neutron stars and supernovae

McDermott, Samuel D.; Reddy, Sanjay; Sen, Srimoyee

doi:10.1103/PhysRevD.99.035013

Title: Deeply bound dibaryon is incompatible with neutron stars and supernovae

Abstract

We study the effect of a dibaryon S in the mass range 1860 < m_S < 2054 MeV, which is heavy enough not to disturb the stability of nuclei and light enough to possibly be cosmologically metastable. Such a deeply bound state can act as a baryon sink in regions of high baryon density and temperature. We find that the ambient conditions encountered inside a newly born neutron star are likely to sustain a sufficient population of hyperons to ensure that a population of S dibaryons can equilibrate in less than a few seconds. This would be catastrophic for the stability of neutron stars and the observation of neutrino emission from the proto-neutron star of Supernova 1987A over ~O(10) s. As a result, a deeply bound dibaryon is therefore incompatible with the observed supernova explosion, unless the cross section for S production is severely suppressed.

Authors:: McDermott, Samuel D.; Reddy, Sanjay; Sen, Srimoyee

Publication Date:: 2019-02-12

Research Org.:: Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Sponsoring Org.:: USDOE Office of Science (SC), High Energy Physics (HEP)

OSTI Identifier:: 1494378

Alternate Identifier(s):: OSTI ID: 1495366

Report Number(s):: arXiv:1809.06765; FERMILAB-PUB-18-490-A
Journal ID: ISSN 2470-0010; PRVDAQ; 035013

Grant/Contract Number:: AC02-07CH11359; FG02-00ER41132

Resource Type:: Published Article

Journal Name:: Physical Review D

Additional Journal Information:: Journal Name: Physical Review D Journal Volume: 99 Journal Issue: 3; Journal ID: ISSN 2470-0010

Publisher:: American Physical Society

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 73 NUCLEAR PHYSICS AND RADIATION PHYSICS

Citation Formats


                    McDermott, Samuel D., Reddy, Sanjay, and Sen, Srimoyee. Deeply bound dibaryon is incompatible with neutron stars and supernovae.  United States: N. p., 2019. 
Web.  doi:10.1103/PhysRevD.99.035013.

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                    McDermott, Samuel D., Reddy, Sanjay, & Sen, Srimoyee. Deeply bound dibaryon is incompatible with neutron stars and supernovae.  United States.  https://doi.org/10.1103/PhysRevD.99.035013

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                    McDermott, Samuel D., Reddy, Sanjay, and Sen, Srimoyee. Tue .  
"Deeply bound dibaryon is incompatible with neutron stars and supernovae".  United States.  https://doi.org/10.1103/PhysRevD.99.035013.

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@article{osti_1494378,

  title        = {Deeply bound dibaryon is incompatible with neutron stars and supernovae},

  author       = {McDermott, Samuel D. and Reddy, Sanjay and Sen, Srimoyee},

  abstractNote = {We study the effect of a dibaryon S in the mass range 1860 < mS < 2054 MeV, which is heavy enough not to disturb the stability of nuclei and light enough to possibly be cosmologically metastable. Such a deeply bound state can act as a baryon sink in regions of high baryon density and temperature. We find that the ambient conditions encountered inside a newly born neutron star are likely to sustain a sufficient population of hyperons to ensure that a population of S dibaryons can equilibrate in less than a few seconds. This would be catastrophic for the stability of neutron stars and the observation of neutrino emission from the proto-neutron star of Supernova 1987A over ~O(10) s. As a result, a deeply bound dibaryon is therefore incompatible with the observed supernova explosion, unless the cross section for S production is severely suppressed.},

  doi          = {10.1103/PhysRevD.99.035013},

  journal      = {Physical Review D},

  number       = 3,

  volume       = 99,

  place        = {United States},

  year         = {2019},

  month        = {2}

}

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Title: Deeply bound dibaryon is incompatible with neutron stars and supernovae

Abstract

Citation Formats

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Λ Λ interaction from relativistic heavy-ion collisions journal, February 2015

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Perhaps a Stable Dihyperon journal, March 1977

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Nuclear and nucleon transitions of the H dibaryon journal, July 2004

Search for the Weak Decay of an H Dibaryon journal, April 1996

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Window in the dark matter exclusion limits journal, October 2005

Constraints on Scattering of keV–TeV Dark Matter with Protons in the Early Universe journal, August 2018

Positive-parity excited baryons in a quark model with hyperfine interactions journal, May 1979

Search for weakly decaying Λ n ‾ and ΛΛ exotic bound states in central Pb–Pb collisions at s NN = 2.76 TeV journal, January 2016

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Systematics of strong interaction radii for hadrons journal, August 1990

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Numerical rates for nucleon-nucleon, axion bremsstrahlung journal, October 1988

Light nuclei and hypernuclei from quantum chromodynamics in the limit of SU(3) flavor symmetry journal, February 2013

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Addendum to “Search for the weak decay of an H dibaryon” journal, August 1997

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Present Constraints on the H-Dibaryon at the Physical Point from Lattice qcd
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Robust constraints and novel gamma-ray signatures of dark matter that interacts strongly with nucleons
journal, June 2018

Mass and lifetime limits on new long-lived particles in 300 GeV/c π− interactions
journal, March 1986

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journal, October 2018

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Evolution of Proto–Neutron Stars
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Nuclear and nucleon transitions of the H dibaryon
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Search for the Weak Decay of an $H$ Dibaryon
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Window in the dark matter exclusion limits
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Constraints on Scattering of keV–TeV Dark Matter with Protons in the Early Universe
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Positive-parity excited baryons in a quark model with hyperfine interactions
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