2018
DOI: 10.1088/1475-7516/2018/04/006
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Cold light dark matter in extended seesaw models

Abstract: We present a thorough discussion of light dark matter produced via freeze-in in two-body decays A → B DM. If A and B are quasi-degenerate, the dark matter particle has a cold spectrum even for keV masses. We show this explicitly by calculating the transfer function that encodes the impact on structure formation. As examples for this setup we study extended seesaw mechanisms with a spontaneously broken global U (1) symmetry, such as the inverse seesaw. The keV-scale pseudo-Goldstone dark matter particle is then… Show more

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Cited by 46 publications
(72 citation statements)
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“…The most stringent limits in this case are Lyman-α forest observations by means of which, limits ranging from m DM 4.09 keV [82] up to m DM 5.3 keV [83] have been obtained for warm DM produced via conventional thermal freeze-out. An intermediate value m DM 4.65 keV [84,85] was used in [86,87] in order to translate this limit to the case of freeze-in DM produced via two-body decays of a parent particle in thermal equilibrium with the plasma . The corresponding limit reads…”
Section: Cosmological Boundsmentioning
confidence: 99%
“…The most stringent limits in this case are Lyman-α forest observations by means of which, limits ranging from m DM 4.09 keV [82] up to m DM 5.3 keV [83] have been obtained for warm DM produced via conventional thermal freeze-out. An intermediate value m DM 4.65 keV [84,85] was used in [86,87] in order to translate this limit to the case of freeze-in DM produced via two-body decays of a parent particle in thermal equilibrium with the plasma . The corresponding limit reads…”
Section: Cosmological Boundsmentioning
confidence: 99%
“…In this region of parameter space Majorons can form DM [27,29,[31][32][33][34][35][36], with a production mechanism that can be unrelated to the small decay couplings [10,27,93,94]. The defining signature of Majoron DM is a flux of neutrinos from DM decay with E ν m J /2 and a known flavor composition [10].…”
Section: B Comparison With Seesaw Observablesmentioning
confidence: 99%
“…For thermal warm dark matter (WDM) these observations place a lower limit on the DM mass in the range m DM 4.09 − 5.3 keV [66][67][68]. In two recent works [69,70] the Lyman-α limit for the case of freeze-in DM produced via two-body decays of a parent particle in thermal equilibrium with the plasma (which is precisely our scenario) has been estimated by comparing the suppression in the linear matter power spectrum from a thermal WDM scenario (with m DM given by the WDM Lyman-α limit, taken to be 4.65 keV [67,71]) to that of the freeze-in scenario. The Lyman-α bound in this case reads…”
Section: Constraints On Dark Matter Freeze-in From Cosmologymentioning
confidence: 99%
“…(3.4)), g i are the number of degrees of freedom of the parent particle A i , the parameter ∆ ij yields the mass splitting between the parent particle and the visible decay product in each channel (e.g. ∆ ij = 1 − m 2 Z /m 2 2 for the decay χ 2 → Zχ 1 ) and η 1.9 [70]. Assuming that freeze-in DM saturates the observed DM relic density, Figure 5 (right) shows the Lyman-α bound on m 1 in the present scenario.…”
Section: Constraints On Dark Matter Freeze-in From Cosmologymentioning
confidence: 99%