Experimental investigation of mode self-locking and stabilization of the repetition frequency of pulses emitted by an He–Ne laser with an absorption cell

We estimate how well we will know the parameters of solar neutrino oscillations after KamLAND and Borexino. The expected error on ∆m 2 is few per-mille in the VO and QVO regions, few per-cent in the LMA region, and around 10% in the LOW region. The expected error on sin 2 2θ is around 5%. KamLAND and Borexino will tell unambiguously which specific new measurement, dedicated to pp solar neutrinos, is able to contribute to the determination of θ and perhaps of ∆m 2 . The present data suggest as more likely outcomes: no measurement, or the total pp rate, or its day/night variation.

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Experimental investigation of mode self-locking and stabilization of the repetition frequency of pulses emitted by an He–Ne laser with an absorption cell

Cited by 2 publications

References 0 publications

Stabilisation of the repetition frequency of femtosecond Ti : Al₂O₃laser pulses

Stabilisation of the repetition frequency of femtosecond Ti : Al₂O₃laser pulses

Femtosecond laser ruler

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Experimental investigation of mode self-locking and stabilization of the repetition frequency of pulses emitted by an He–Ne laser with an absorption cell

Cited by 2 publications

References 0 publications

Stabilisation of the repetition frequency of femtosecond Ti : Al2O3laser pulses

Stabilisation of the repetition frequency of femtosecond Ti : Al2O3laser pulses

Femtosecond laser ruler

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Product

Resources

About

Stabilisation of the repetition frequency of femtosecond Ti : Al₂O₃laser pulses

Stabilisation of the repetition frequency of femtosecond Ti : Al₂O₃laser pulses