Cosmic Explosions, Life in the Universe, and the Cosmological Constant.

Gamma-ray bursts (GRBs) are copious sources of gamma rays whose interaction with a planetary atmosphere can pose a threat to complex life. Using recent determinations of their rate and probability of causing massive extinction, we explore what types of universes are most likely to harbor advanced forms of life. We use cosmological N-body simulations to determine at what time and for what value of the cosmological constant (Λ) the chances of life being unaffected by cosmic explosions are maximized. Life survival to GRBs favors Lambda-dominated universes. Within a cold dark matter model with a cosmological constant, the likelihood of life survival to GRBs is governed by the value of Λ and the age of the Universe. We find that we seem to live in a favorable point in this parameter space that minimizes the exposure to cosmic explosions, yet maximizes the number of main sequence (hydrogen-burning) stars around which advanced life forms can exist.

Unscreening Modified Gravity in the Matter Power Spectrum.

Viable modifications of gravity that may produce cosmic acceleration need to be screened in high-density regions such as the Solar System, where general relativity is well tested. Screening mechanisms also prevent strong anomalies in the large-scale structure and limit the constraints that can be inferred on these gravity models from cosmology. We find that by suppressing the contribution of the screened high-density regions in the matter power spectrum, allowing a greater contribution of unscreened low densities, modified gravity models can be more readily discriminated from the concordance cosmology. Moreover, by variation of density thresholds, degeneracies with other effects may be dealt with more adequately. Specializing to chameleon gravity as a worked example for screening in modified gravity, employing N-body simulations of f(R) models and the halo model of chameleon theories, we demonstrate the effectiveness of this method. We find that a percent-level measurement of the clipped power at k<0.3h/Mpc can yield constraints on chameleon models that are more stringent than what is inferred from Solar System tests or distance indicators in unscreened dwarf galaxies. Finally, we verify that our method is also applicable to the Vainshtein mechanism.

Clipping the cosmos: the bias and bispectrum of large scale structure.

A large fraction of the information collected by cosmological surveys is simply discarded to avoid length scales which are difficult to model theoretically. We introduce a new technique which enables the extraction of useful information from the bispectrum of galaxies well beyond the conventional limits of perturbation theory. Our results strongly suggest that this method increases the range of scales where the relation between the bispectrum and power spectrum in tree-level perturbation theory may be applied, from k(max) ∼ 0.1 to ∼0.7 hMpc(-1). This leads to correspondingly large improvements in the determination of galaxy bias. Since the clipped matter power spectrum closely follows the linear power spectrum, there is the potential to use this technique to probe the growth rate of linear perturbations and confront theories of modified gravity with observation.

Arrhythmogenic substrate and its modification by nicorandil in a murine model of long QT type 3 syndrome.

The gain-of-function Scn5a+/DeltaKPQ mutation in the cardiac Na(+) channel causes human long QT type 3 syndrome (LQT3) associated with ventricular arrhythmogenesis. The K(ATP) channel-opener nicorandil (20muM) significantly reduced arrhythmic incidence in Langendorff-perfused Scn5a+/Delta hearts during programmed electrical stimulation; wild-types (WTs) showed a total absence of arrhythmogenicity. These observations precisely correlated with alterations in recently established criteria for re-entrant excitation reflected in: (1) shortened left-ventricular epicardial but not endocardial monophasic action potential durations at 90% repolarization (APD(90)) that (2) restored transmural repolarization gradients, DeltaAPD(90). Scn5a+/Delta hearts showed longer epicardial but not endocardial APD(90)s, giving shorter DeltaAPD(90)s than WT hearts. Nicorandil reduced epicardial APD(90) in both Scn5a+/Delta and WT hearts thereby increasing DeltaAPD(90). (3) Reduced epicardial critical intervals for re-excitation; Scn5a+/Delta hearts showed greater differences between APD(90) and ventricular effective refractory period than WT hearts that were reduced by nicorandil. (4) Reduced APD(90) alternans. Scn5a+/Delta hearts showed greater epicardial and endocardial alternans than WTs, which increased with pacing rate. Nicorandil reduced these in Scn5a+/Delta hearts to levels indistinguishable from untreated WTs. (5) Flattened restitution curves. Scn5a+/Delta hearts showed larger epicardial and endocardial critical diastolic intervals than WT hearts. Nicorandil decreased these in Scn5a+/Delta and WT hearts. The presence or absence of arrhythmogenesis in Scn5a+/Delta and WT hearts thus agreed with previously established criteria for re-entrant excitation, and alterations in these precisely correlated with the corresponding antiarrhythmic effects of nicorandil. Together these findings implicate spatial and temporal re-entrant mechanisms in arrhythmogenesis in LQT3 and their reversal by nicorandil.