Introduction to Particle Physics
How much energy is released when an electron and a positron at rest annihilate each other? (For particle masses, see Table 11.1.)
Chapter 16 – Star Birth Stellar Evolution ● Stars are like ppl in that they are born, grow up, mature & die ● Star’s mass determines what life path i t will take ● We divide all stars into 3 groups: o Low mass ( .08 of sun M) ● H-R diagram makes u seful ap ● Life o f ny star battle f 2 forces: o Gravity vs. “something else” ● Gravity always wants t o collapse tar o The “ something else” holds up tar o Type i s st s defined y “something e lse” ● Remember: Newton’s law of gravity o Amnt. Of gravitational force depends o n mass o Gravitational potential energy into heat as star collapses The tellar Womb ● Stars born d eep in olecular clouds o Cold (10 – 0 ) dense nebulae o So cold that H2 can exist ● Cold cloud c an ragment Stellar Gestation ● Something happens to perturb a molecular cloud & make it begin to fragment ● As core of as collapses, t heats up o Radiates infrared from its surface o Protostar ● Protostar collapses until its core reaches 10 K