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2016
DOI: 10.1103/physrevd.93.033002
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Asymmetric dark matter and effective number of neutrinos

Abstract: We study the effect of the MeV-scale asymmetric dark matter annihilation on the effective number of neutrinos $N_{\rm eff}$ at the epoch of the big bang nucleosynthesis. If the asymmetric dark matter $\chi$ couples more strongly to the neutrinos $\nu$ than to the photons $\gamma$ and electrons $e^-$, $\Gamma_{\chi\gamma, \chi e} \ll \Gamma_{\chi\nu}$, or $\Gamma_{\chi\gamma, \chi e} \gg \Gamma_{\chi\nu}$, the lower mass limit on the asymmetric dark matter is about $18$ MeV for $N_{\rm eff}\simeq 3.0$.Comment: … Show more

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Cited by 6 publications
(8 citation statements)
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“…Because the nearly degenerated mass pattern |m 1 | ∼ |m 2 | ∼ |m 3 | is compatible with observed data for the two zero flavor textures, [15][16][17][18][19] we require rank(m D ) = rank(m D ) = 3 for the Dirac mass matrix: e.g., if we allow rank(m D ) < 3, at least one of the neutrino masses m 1 , m 2 , m 3 should vanish and we cannot guarantee the nearly degenerate mass pattern. The Dirac mass matrix with all zero entries in a row or a column such as and with same row or same column such as…”
Section: Allowed Combinations Of Four Zerossupporting
confidence: 77%
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“…Because the nearly degenerated mass pattern |m 1 | ∼ |m 2 | ∼ |m 3 | is compatible with observed data for the two zero flavor textures, [15][16][17][18][19] we require rank(m D ) = rank(m D ) = 3 for the Dirac mass matrix: e.g., if we allow rank(m D ) < 3, at least one of the neutrino masses m 1 , m 2 , m 3 should vanish and we cannot guarantee the nearly degenerate mass pattern. The Dirac mass matrix with all zero entries in a row or a column such as and with same row or same column such as…”
Section: Allowed Combinations Of Four Zerossupporting
confidence: 77%
“…[26][27][28] In the two zero flavor neutrino mass matrix scheme, there are 15 possible combinations of two vanishing independent elements in the flavor neutrino mass matrix. If we require a nonvanishing Majorana effective mass M ee for the neutrinoless double beta decay, the viable textures are the following [15][16][17][18][19]…”
Section: Seesaw Modelmentioning
confidence: 99%
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“…These textures have been extensively studied [5,[14][15][16][17][18][19][20][21][22][23][24][25][26][27][28][29]. Here for completeness we present some results and give an estimate of the radiative correction for the neutrinoless double beta decay effective mass parameter.…”
Section: A Phenomenologymentioning
confidence: 99%
“…In paricular, the phenomenology of one-zero and two-zero textures was studied in Refs. [57][58][59][60] and [61][62][63][64][65][66][67][68][69][70][71][72][73][74], respectively. Also, the experimental potential of probing the texture-zero models has been discussed.…”
Section: (D')mentioning
confidence: 99%