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1.
J Neurosci ; 34(17): 5747-53, 2014 Apr 23.
Artigo em Inglês | MEDLINE | ID: mdl-24760835

RESUMO

Chronic pain is often associated with sexual dysfunction, suggesting that pain can reduce libido. We find that inflammatory pain reduces sexual motivation, measured via mounting behavior and/or proximity in a paced mating paradigm, in female but not male laboratory mice. Pain was produced by injection of inflammogens zymosan A (0.5 mg/ml) or λ-carrageenan (2%) into genital or nongenital (hind paw, tail, cheek) regions. Sexual behavior was significantly reduced in female mice experiencing pain (in all combinations); male mice similarly treated displayed unimpeded sexual motivation. Pain-induced reductions in female sexual behavior were observed in the absence of sex differences in pain-related behavior, and could be rescued by the analgesic, pregabalin, and the libido-enhancing drugs, apomorphine and melanotan-II. These findings suggest that the well known context sensitivity of the human female libido can be explained by evolutionary rather than sociocultural factors, as female mice can be similarly affected.


Assuntos
Libido/fisiologia , Motivação/fisiologia , Dor/psicologia , Comportamento Sexual Animal/fisiologia , Analgésicos/farmacologia , Animais , Apomorfina/farmacologia , Carragenina , Agonistas de Dopamina/farmacologia , Feminino , Libido/efeitos dos fármacos , Masculino , Camundongos , Motivação/efeitos dos fármacos , Dor/induzido quimicamente , Peptídeos Cíclicos/farmacologia , Pregabalina , Fatores Sexuais , Comportamento Sexual Animal/efeitos dos fármacos , Zimosan , alfa-MSH/análogos & derivados , alfa-MSH/farmacologia , Ácido gama-Aminobutírico/análogos & derivados , Ácido gama-Aminobutírico/farmacologia
2.
Proc Natl Acad Sci U S A ; 110(21): 8453-8, 2013 May 21.
Artigo em Inglês | MEDLINE | ID: mdl-23650386

RESUMO

The lifetime of the ancient lunar core dynamo has implications for its power source and the mechanism of field generation. Here, we report analyses of two 3.56-Gy-old mare basalts demonstrating that they were magnetized in a stable and surprisingly intense dynamo magnetic field of at least ~13 µT. These data extend the known lifetime of the lunar dynamo by ~160 My and indicate that the field was likely continuously active until well after the final large basin-forming impact. This likely excludes impact-driven changes in rotation rate as the source of the dynamo at this time in lunar history. Rather, our results require a persistent power source like precession of the lunar mantle or a compositional convection dynamo.

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