The Intersectionality of Intimate Partner Violence in the Black Community

To adequately address intimate partner violence in the black community in the USA, it is imperative to discuss historical oppression and examine how intersecting realities influence intimate partner/gender-based violence and individual, community, and systemic responses. Institutionalized and internalized oppression through racism, sexism, classism, homophobia, xenophobia, religious subjugation, etc., perpetuates unrecognized, unaddressed, and denied traumatic experiences for black survivors. One of the leading causes of death for black women aged 15–35 is intimate partner violence. Black women are almost three times more likely than white women to be killed by an intimate partner. This chapter will explore why culturally specific, trauma-informed practices are essential for holistic responses. For a black survivor, oppression, implicit/explicit bias, and racial loyalty/collectivism directly impact how female survivors perceive, react to, and report intimate partner violence. Racism and stereotypes continue to contribute to the failure of the legal systems, crisis services, and other programs to provide adequate resources and assistance to black survivors. Survivors who are foreign-born Africans, Afro Caribbeans, and Afro Latinas experience limited access to services in their first languages and/or limited interpreters who speak the native language, fear of interacting with systems and deportation, and little cultural understanding and empathy from service providers. We will provide promising practices, guiding principles, and culturally specific resources to illuminate the opportunities that exist to support the resiliency, autonomy, and self-determination of black survivors

Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M _⊙ Compact Object and a Neutron Star

Abstract We report the observation of a coalescing compact binary with component masses 2.5–4.5 M ⊙ and 1.2–2.0 M ⊙ (all measurements quoted at the 90% credible level). The gravitational-wave signal GW230529_181500 was observed during the fourth observing run of the LIGO–Virgo–KAGRA detector network on 2023 May 29 by the LIGO Livingston observatory. The primary component of the source has a mass less than 5 M ⊙ at 99% credibility. We cannot definitively determine from gravitational-wave data alone whether either component of the source is a neutron star or a black hole. However, given existing estimates of the maximum neutron star mass, we find the most probable interpretation of the source to be the coalescence of a neutron star with a black hole that has a mass between the most massive neutron stars and the least massive black holes observed in the Galaxy. We provisionally estimate a merger rate density of 55 − 47 + 127 Gpc − 3 yr − 1 for compact binary coalescences with properties similar to the source of GW230529_181500; assuming that the source is a neutron star–black hole merger, GW230529_181500-like sources may make up the majority of neutron star–black hole coalescences. The discovery of this system implies an increase in the expected rate of neutron star–black hole mergers with electromagnetic counterparts and provides further evidence for compact objects existing within the purported lower mass gap.</jats:p