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0002014v1
2
teresting to verify this [the existence of a KT transition for $$X Y$$ models on a fractal lattice]”. Yet we do not see the relevance of such an obvious claim. We disagree however with the authors of [1] when they say “our ar- gument does not depend on the existence of such a transition on that particular percolating ...
<p>teresting to verify this [the existence of a KT transition for $$X Y$$ models on a fractal lattice]”. Yet we do not see the relevance of such an obvious claim.</p> <p>We disagree however with the authors of [1] when they say “our ar- gument does not depend on the existence of such a transition on that particular per...
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0002014v1
0
# Reply to A. Patrascioiu’s and E. Seiler’s comment on our paper # Percolation properties of the 2D Heisenberg model B. Allés $$\mathrm{a}$$ , J. J. Alonso $$\mathrm{b}$$ , C. Criado $$\mathrm{b}$$ , M. Pepe $$\mathrm{c}$$ $$\mathrm{a}$$ Dipartimento di Fisica, Universita di Milano-Bicocca and INFN Sezione di Milano...
<h1>Reply to A. Patrascioiu’s and E. Seiler’s comment on our paper</h1> <h1>Percolation properties of the 2D Heisenberg model</h1> <p>B. Allés $$\mathrm{a}$$ , J. J. Alonso $$\mathrm{b}$$ , C. Criado $$\mathrm{b}$$ , M. Pepe $$\mathrm{c}$$</p> <p>$$\mathrm{a}$$ Dipartimento di Fisica, Universita di Milano-Bicocca and I...
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0002004v1
0
# Three generation neutrino mixing is compatible with all experiments B. Hoeneisen and C. Marı´n Universidad San Francisco de Quito 2 February 2000 # Abstract We consider the minimal extension of the Standard Model with three generations of massive neutrinos that mix. We then determine the parameters of the model t...
<h1>Three generation neutrino mixing is compatible with all experiments</h1> <p>B. Hoeneisen and C. Marı´n</p> <p>Universidad San Francisco de Quito 2 February 2000</p> <h1>Abstract</h1> <p>We consider the minimal extension of the Standard Model with three generations of massive neutrinos that mix. We then determine th...
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0002004v1
4
with 116 degrees of freedom, including the 8 discussed earlier plus the 108 measurements by the Homestake Collaboration from 1970.281 to 1994.388[12] we obtain the allowed region shown in Figure 2. The reliability of $$M_{2}^{2}\mathrm{~-~}M_{1}^{2}$$ depends on the correctness of the error as- signed to the Homestake...
<p>with 116 degrees of freedom, including the 8 discussed earlier plus the 108 measurements by the Homestake Collaboration from 1970.281 to 1994.388[12] we obtain the allowed region shown in Figure 2.</p> <p>The reliability of $$M_{2}^{2}\mathrm{~-~}M_{1}^{2}$$ depends on the correctness of the error as- signed to the ...
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0002014v1
1
"test was cited in [3] but the details of the numerics (temperature, size of\nthe lattice, etc.) and(...TRUNCATED)
"<p>test was cited in [3] but the details of the numerics (temperature, size of\nthe lattice, etc.) (...TRUNCATED)
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0002004v1
3
"Table 3: Limits on the mixing probabilities from astrophysical, accelerator\nand reactor experiment(...TRUNCATED)
"<p>Table 3: Limits on the mixing probabilities from astrophysical, accelerator\nand reactor experim(...TRUNCATED)
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[612.0, 792.0]
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0002004v1
1
"Table 1: Observed solar electron-type neutrino flux, compared to the Stan-\ndard Solar Model (SSM) (...TRUNCATED)
"<p>Table 1: Observed solar electron-type neutrino flux, compared to the Stan-\ndard Solar Model (SS(...TRUNCATED)
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0002004v1
2
"Table 2: Ratio of the numbers of observed and predicted electron-type and\nmuon-type neutrinos as a(...TRUNCATED)
"<p>Table 2: Ratio of the numbers of observed and predicted electron-type and\nmuon-type neutrinos a(...TRUNCATED)
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0002004v1
6
"[5] KAMIOKANDE Collab., Y. Fukuda et al., Phys. Rev. Lett. 77 (1996)\n1683\n[6] Super-Kamiokande Co(...TRUNCATED)
"<p>[5] KAMIOKANDE Collab., Y. Fukuda et al., Phys. Rev. Lett. 77 (1996)\n1683\n[6] Super-Kamiokande(...TRUNCATED)
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0002004v1
5
"$$T_{f}$$ : their temperature has lagged below the temperature of photons due to\nthe anihilation o(...TRUNCATED)
"<p>$$T_{f}$$ : their temperature has lagged below the temperature of photons due to\nthe anihilatio(...TRUNCATED)
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