Materia oscura fredda (Italian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Materia oscura fredda" in Italian language version.

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11harvard.edu

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1osti.gov

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arxiv.org

Francesca Chadha-Day, John Ellis e David J. E. Marsh, Axion dark matter: What is it and why now?, in Science Advances, vol. 8, n. 8, 23 febbraio 2022, pp. eabj3618, Bibcode:2022SciA....8J3618C, DOI:10.1126/sciadv.abj3618, PMC 8865781, PMID 35196098, arXiv:2105.01406.
B.J. Carr, New cosmological constraints on primordial black holes, in Physical Review D, vol. 81, n. 10, maggio 2010, p. 104019, Bibcode:2010PhRvD..81j4019C, DOI:10.1103/PhysRevD.81.104019, arXiv:0912.5297.
Gianfranco Bertone, Dan Hooper e Joseph Silk, Particle dark matter: evidence, candidates and constraints, in Physics Reports, vol. 405, 5–6, gennaio 2005, pp. 279–390, Bibcode:2005PhR...405..279B, DOI:10.1016/j.physrep.2004.08.031, arXiv:hep-ph/0404175.
Katherine Garrett e Gintaras Dūda, Dark Matter: A Primer, in Advances in Astronomy, vol. 2011, 2011, p. 968283, Bibcode:2011AdAst2011E...8G, DOI:10.1155/2011/968283, arXiv:1006.2483.
«MACHOs can only account for a very small percentage of the nonluminous mass in our galaxy, revealing that most dark matter cannot be strongly concentrated or exist in the form of baryonic astrophysical objects. Although microlensing surveys rule out baryonic objects like brown dwarfs, black holes, and neutron stars in our galactic halo, can other forms of baryonic matter make up the bulk of dark matter? The answer, surprisingly, is ‘no’ ...»
Keith A. Olive, TASI lectures on dark matter, in Physics, vol. 54, 2003, p. 21, Bibcode:2003astro.ph..1505O, arXiv:astro-ph/0301505.
R. Bernabei et al., Dark Matter search, in Rivista del Nuovo Cimento, vol. 26, n. 1, 2003, p. 1, Bibcode:2003NCimR..26a...1B, arXiv:astro-ph/0307403.
R. Bernabei et al., The DAMA/LIBRA apparatus, in Nuclear Instruments and Methods in Physics Research A, vol. 592, n. 1, 2008, pp. 297, Bibcode:2008NIMPA.592..297B, DOI:10.1016/j.nima.2008.04.082, arXiv:0804.2738.

doi.org

dx.doi.org

P. J. E. Peebles, Large-scale background temperature and mass fluctuations due to scale-invariant primeval perturbations, in The Astrophysical Journal, vol. 263, dicembre 1982, pp. L1, Bibcode:1982ApJ...263L...1P, DOI:10.1086/183911.
J. R. Bond, A. S. Szalay e M. S. Turner, Formation of galaxies in a gravitino-dominated universe, in Physical Review Letters, vol. 48, n. 23, 1982, pp. 1636–1639, Bibcode:1982PhRvL..48.1636B, DOI:10.1103/PhysRevLett.48.1636.
George R. Blumenthal, Heinz Pagels e Joel R. Primack, Galaxy formation by dissipationless particles heavier than neutrinos, in Nature, vol. 299, n. 5878, 2 settembre 1982, pp. 37–38, Bibcode:1982Natur.299...37B, DOI:10.1038/299037a0.
G. R. Blumenthal, S. M. Faber, J. R. Primack e M. J. Rees, Formation of galaxies and large-scale structure with cold dark matter, in Nature, vol. 311, n. 517, 1984, pp. 517–525, Bibcode:1984Natur.311..517B, DOI:10.1038/311517a0, OSTI 1447148.
Francesca Chadha-Day, John Ellis e David J. E. Marsh, Axion dark matter: What is it and why now?, in Science Advances, vol. 8, n. 8, 23 febbraio 2022, pp. eabj3618, Bibcode:2022SciA....8J3618C, DOI:10.1126/sciadv.abj3618, PMC 8865781, PMID 35196098, arXiv:2105.01406.
B.J. Carr, New cosmological constraints on primordial black holes, in Physical Review D, vol. 81, n. 10, maggio 2010, p. 104019, Bibcode:2010PhRvD..81j4019C, DOI:10.1103/PhysRevD.81.104019, arXiv:0912.5297.
Gianfranco Bertone, Dan Hooper e Joseph Silk, Particle dark matter: evidence, candidates and constraints, in Physics Reports, vol. 405, 5–6, gennaio 2005, pp. 279–390, Bibcode:2005PhR...405..279B, DOI:10.1016/j.physrep.2004.08.031, arXiv:hep-ph/0404175.
Katherine Garrett e Gintaras Dūda, Dark Matter: A Primer, in Advances in Astronomy, vol. 2011, 2011, p. 968283, Bibcode:2011AdAst2011E...8G, DOI:10.1155/2011/968283, arXiv:1006.2483.
«MACHOs can only account for a very small percentage of the nonluminous mass in our galaxy, revealing that most dark matter cannot be strongly concentrated or exist in the form of baryonic astrophysical objects. Although microlensing surveys rule out baryonic objects like brown dwarfs, black holes, and neutron stars in our galactic halo, can other forms of baryonic matter make up the bulk of dark matter? The answer, surprisingly, is ‘no’ ...»
R. Bernabei et al., The DAMA/LIBRA apparatus, in Nuclear Instruments and Methods in Physics Research A, vol. 592, n. 1, 2008, pp. 297, Bibcode:2008NIMPA.592..297B, DOI:10.1016/j.nima.2008.04.082, arXiv:0804.2738.

harvard.edu

adsabs.harvard.edu

P. J. E. Peebles, Large-scale background temperature and mass fluctuations due to scale-invariant primeval perturbations, in The Astrophysical Journal, vol. 263, dicembre 1982, pp. L1, Bibcode:1982ApJ...263L...1P, DOI:10.1086/183911.
J. R. Bond, A. S. Szalay e M. S. Turner, Formation of galaxies in a gravitino-dominated universe, in Physical Review Letters, vol. 48, n. 23, 1982, pp. 1636–1639, Bibcode:1982PhRvL..48.1636B, DOI:10.1103/PhysRevLett.48.1636.
George R. Blumenthal, Heinz Pagels e Joel R. Primack, Galaxy formation by dissipationless particles heavier than neutrinos, in Nature, vol. 299, n. 5878, 2 settembre 1982, pp. 37–38, Bibcode:1982Natur.299...37B, DOI:10.1038/299037a0.
G. R. Blumenthal, S. M. Faber, J. R. Primack e M. J. Rees, Formation of galaxies and large-scale structure with cold dark matter, in Nature, vol. 311, n. 517, 1984, pp. 517–525, Bibcode:1984Natur.311..517B, DOI:10.1038/311517a0, OSTI 1447148.
Francesca Chadha-Day, John Ellis e David J. E. Marsh, Axion dark matter: What is it and why now?, in Science Advances, vol. 8, n. 8, 23 febbraio 2022, pp. eabj3618, Bibcode:2022SciA....8J3618C, DOI:10.1126/sciadv.abj3618, PMC 8865781, PMID 35196098, arXiv:2105.01406.
B.J. Carr, New cosmological constraints on primordial black holes, in Physical Review D, vol. 81, n. 10, maggio 2010, p. 104019, Bibcode:2010PhRvD..81j4019C, DOI:10.1103/PhysRevD.81.104019, arXiv:0912.5297.
Gianfranco Bertone, Dan Hooper e Joseph Silk, Particle dark matter: evidence, candidates and constraints, in Physics Reports, vol. 405, 5–6, gennaio 2005, pp. 279–390, Bibcode:2005PhR...405..279B, DOI:10.1016/j.physrep.2004.08.031, arXiv:hep-ph/0404175.
Katherine Garrett e Gintaras Dūda, Dark Matter: A Primer, in Advances in Astronomy, vol. 2011, 2011, p. 968283, Bibcode:2011AdAst2011E...8G, DOI:10.1155/2011/968283, arXiv:1006.2483.
«MACHOs can only account for a very small percentage of the nonluminous mass in our galaxy, revealing that most dark matter cannot be strongly concentrated or exist in the form of baryonic astrophysical objects. Although microlensing surveys rule out baryonic objects like brown dwarfs, black holes, and neutron stars in our galactic halo, can other forms of baryonic matter make up the bulk of dark matter? The answer, surprisingly, is ‘no’ ...»
Keith A. Olive, TASI lectures on dark matter, in Physics, vol. 54, 2003, p. 21, Bibcode:2003astro.ph..1505O, arXiv:astro-ph/0301505.
R. Bernabei et al., Dark Matter search, in Rivista del Nuovo Cimento, vol. 26, n. 1, 2003, p. 1, Bibcode:2003NCimR..26a...1B, arXiv:astro-ph/0307403.
R. Bernabei et al., The DAMA/LIBRA apparatus, in Nuclear Instruments and Methods in Physics Research A, vol. 592, n. 1, 2008, pp. 297, Bibcode:2008NIMPA.592..297B, DOI:10.1016/j.nima.2008.04.082, arXiv:0804.2738.

nih.gov

ncbi.nlm.nih.gov

Francesca Chadha-Day, John Ellis e David J. E. Marsh, Axion dark matter: What is it and why now?, in Science Advances, vol. 8, n. 8, 23 febbraio 2022, pp. eabj3618, Bibcode:2022SciA....8J3618C, DOI:10.1126/sciadv.abj3618, PMC 8865781, PMID 35196098, arXiv:2105.01406.

oadoi.org

P. J. E. Peebles, Large-scale background temperature and mass fluctuations due to scale-invariant primeval perturbations, in The Astrophysical Journal, vol. 263, dicembre 1982, pp. L1, Bibcode:1982ApJ...263L...1P, DOI:10.1086/183911.
J. R. Bond, A. S. Szalay e M. S. Turner, Formation of galaxies in a gravitino-dominated universe, in Physical Review Letters, vol. 48, n. 23, 1982, pp. 1636–1639, Bibcode:1982PhRvL..48.1636B, DOI:10.1103/PhysRevLett.48.1636.
George R. Blumenthal, Heinz Pagels e Joel R. Primack, Galaxy formation by dissipationless particles heavier than neutrinos, in Nature, vol. 299, n. 5878, 2 settembre 1982, pp. 37–38, Bibcode:1982Natur.299...37B, DOI:10.1038/299037a0.
G. R. Blumenthal, S. M. Faber, J. R. Primack e M. J. Rees, Formation of galaxies and large-scale structure with cold dark matter, in Nature, vol. 311, n. 517, 1984, pp. 517–525, Bibcode:1984Natur.311..517B, DOI:10.1038/311517a0, OSTI 1447148.
B.J. Carr, New cosmological constraints on primordial black holes, in Physical Review D, vol. 81, n. 10, maggio 2010, p. 104019, Bibcode:2010PhRvD..81j4019C, DOI:10.1103/PhysRevD.81.104019, arXiv:0912.5297.
Gianfranco Bertone, Dan Hooper e Joseph Silk, Particle dark matter: evidence, candidates and constraints, in Physics Reports, vol. 405, 5–6, gennaio 2005, pp. 279–390, Bibcode:2005PhR...405..279B, DOI:10.1016/j.physrep.2004.08.031, arXiv:hep-ph/0404175.
Katherine Garrett e Gintaras Dūda, Dark Matter: A Primer, in Advances in Astronomy, vol. 2011, 2011, p. 968283, Bibcode:2011AdAst2011E...8G, DOI:10.1155/2011/968283, arXiv:1006.2483.
«MACHOs can only account for a very small percentage of the nonluminous mass in our galaxy, revealing that most dark matter cannot be strongly concentrated or exist in the form of baryonic astrophysical objects. Although microlensing surveys rule out baryonic objects like brown dwarfs, black holes, and neutron stars in our galactic halo, can other forms of baryonic matter make up the bulk of dark matter? The answer, surprisingly, is ‘no’ ...»
R. Bernabei et al., The DAMA/LIBRA apparatus, in Nuclear Instruments and Methods in Physics Research A, vol. 592, n. 1, 2008, pp. 297, Bibcode:2008NIMPA.592..297B, DOI:10.1016/j.nima.2008.04.082, arXiv:0804.2738.

osti.gov

G. R. Blumenthal, S. M. Faber, J. R. Primack e M. J. Rees, Formation of galaxies and large-scale structure with cold dark matter, in Nature, vol. 311, n. 517, 1984, pp. 517–525, Bibcode:1984Natur.311..517B, DOI:10.1038/311517a0, OSTI 1447148.