By Patricia C. Wrede
Drinn isn't really a secure position to be a witch. Ranira understands that higher than so much, for while she used to be only a baby, the temple guards burned her mom and dad on the stake for training magic.
Now an indentured servant for a brutal innkeeper, she lives each day with the disgrace of her parents’ alleged crime. there's no worse time to go to Drinn than throughout the Midwinter pageant, while the town gates are sealed in order that no outsider can witness the temple’s mystery rituals. And at Ranira’s resort, 3 site visitors have overstayed their welcome.
Attempting to guard Ranira from her master’s cruelty, the 3 exhibit their magical powers and allure the eye of the temple guards. Now, to save lots of her new buddies from yes demise, Ranira needs to unharness the ability that price her mom and dad their lives.
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Additional resources for Daughter of Witches (Lyra, Book 2)
Observatories (dashed and dash-dotted lines, respectively). The latter are adapted from , for Majorana dark matter particle . . . . . . . . 157 . 158 . 160 . 161 . 161 . 162 . 162 . 163 . 5 List of Figures Artist’s impression of the CTA, with telescopes of different sizes visible. Credit G. Pérez/IAC/SMM . . . . . . . The integral sensitivity for CTA from MC simulations, together with the sensitivity in comparable conditions (50 h for IACTs, 1 year for Fermi-LAT and HAWC) for other gamma-ray observatories.
The dominant final states are composed by heavy particles, like τ + τ − , bb¯ and t t¯ (for sufficiently high masses). • Photons: direct annihilation into photons can occur at one loop level, as χ χ → γ X , where X = γ , Z or h. Such process is strongly suppressed, but not impossible; photons produced this way would be detected as sharp lines at energies E γ ≈ m χ (1 − m 2X /4m 2χ ) (Sect. 3), representing an undoubtable evidence of dark matter detection. Photons can also be produced in the so-called internal bremsstrahlung : if neutralinos annihilate into leptons, the annihilation exchange particle is a charged sparticle that can emit a photon.
L. upper limits on hσ ann vi as a function of mχ , for bb (top), τ þ τÀ (middle) and W þ W À channels (bottom), estimated for 150 h of Segue 1 observations with CTA, calculated with the full likelihood (full black lines) and with the conventional approach (dashed black lines). Also shown are the exclusion curves from MAGIC (obtained from this work Sect. 1, full blue, red and green lines, for the considered channels, respectively) and from Fermi-LAT (long-dashed lines, same color coding, ) .