UVA induces retinal photoreceptor cell death via receptor interacting protein 3 kinase mediated necroptosis

Ultraviolet light A (UVA) is the only UV light that reaches the retina and can cause indirect damage to DNA via absorption of photons by non-DNA chromophores. Previous studies demonstrate that UVA generates reactive oxygen species (ROS) and leads to programmed cell death. Programmed cell death (PCD) has been implicated in numerous ophthalmologic diseases. Here, we investigated receptor interacting protein 1 and 3 (RIPK1 and RIPK3) kinases, key signaling molecules of PCD, in UVA-induced photoreceptor injury using in vitro and ex vivo models. UVA irradiation activated RIPK3 but not RIPK1 and mediated necroptosis through MLKL that lie downstream of RIPK3 and induced apoptosis through increased oxidative stress. Moreover, RIPK3 but not RIPK1 inhibition suppresses UVA-induced cell death along with the downregulation of MLKL and attenuates the levels of oxidative stress and DNA fragmentation. In conclusion, these results identify RIPK3, not RIPK1, as a critical regulator of UVA-induced necroptosis cell death in photoreceptors and highlight RIPK3 potential as a neuroprotective target.This work was supported by the Yeatts Family Foundation (D.G.V.); Monte J. Wallace (D.G.V.); 2013 Macula Society Research Grant Award (to D.G.V.); a Physician Scientist Award (to D.G.V.); unrestricted grant from the Research to Prevent Blindness Foundation (to J.W.M. and D.G.V.); National Eye Institute (NEI) R21EY023079-01/A1 (to D.G.V.); NEI Grant EY014104 (Massachusetts Eye and Ear Infirmary Core Grant) (to D.G.V.); Loeffler Family Fund (D.G.V.); R01EY025362-01 (to D.G.V.); ARI Young Investigator Award (to D.G.V.); Foundation Lions Eye Research Fund (D.G.V.); NIH NEI Core Grant P30EY003790 (to D.G.V.); Loeffler Family Fund (to D.G.V.); ARI Young Investigator Award (to D.G.V.). Shenzhen Science and Technology Program (Grant No. JCYJ20220530153607015); Shenzhen Science and Technology Program (Grant No. JCYJ20220531094004010); Shenzhen-Hong Kong Co-financing Project (Grant No. SGDX20190920110403741); Guangdong Basic and Applied Basic Research Foundation (No. 2022A1515012326); Shenzhen Science and Technology Program (Grant No. JSGG20201102174200001); Shenzhen Key Medical Discipline Construction Fund (No. SZXK038); Sanming Project of Medicine in Shenzhen (No. SZSM202011015); Shenzhen Fund for Guangdong Provincial High level Clinical Key Specialties (No. SZGSP014); National Natural Science Foundation of China (No. 82271103)

Search for eccentric black hole coalescences during the third observing run of LIGO and Virgo

Despite the growing number of binary black hole coalescences confidently observed through gravitational waves so far, the astrophysical origin of these binaries remains uncertain. Orbital eccentricity is one of the clearest tracers of binary formation channels. Identifying binary eccentricity, however, remains challenging due to the limited availability of gravitational waveforms that include the effects of eccentricity. Here, we present observational results for a waveform-independent search sensitive to eccentric black hole coalescences, covering the third observing run (O3) of the LIGO and Virgo detectors. We identified no new high-significance candidates beyond those that have already been identified with searches focusing on quasi-circular binaries. We determine the sensitivity of our search to high-mass (total source-frame mass M > 70 M⊙) binaries covering eccentricities up to 0.3 at 15 Hz emitted gravitational-wave frequency, and use this to compare model predictions to search results. Assuming all detections are indeed quasi-circular, for our fiducial population model, we place a conservative upper limit for the merger rate density of high-mass binaries with eccentricities 0 < e ≤ 0.3 at 16.9 Gpc−3 yr−1 at the 90% confidence level