2014
DOI: 10.1016/j.nima.2013.08.030
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The prototype GAPS (pGAPS) experiment

Abstract: The General Antiparticle Spectrometer (GAPS) experiment is a novel approach for the detection of cosmic ray antiparticles. A prototype GAPS experiment (pGAPS) was successfully flown on a high-altitude balloon in June of 2012. The goals of the pGAPS experiment were: to test the operation of lithium drifted silicon (Si(Li)) detectors at balloon altitudes, to validate the thermal model and cooling concept needed for engineering of a full-size GAPS instrument, and to characterize cosmic ray and X-ray backgrounds. … Show more

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Cited by 28 publications
(29 citation statements)
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“…Big-bang nucleosynthesis is the dominant natural source of deuterons [27] and, in the absence of baryogenesis, one could assume that the same holds for antideuterons. These antinuclei and even heavier antinuclei can also be produced in pp and pA collisions in interstellar space, representing a background source in the searches for segregated primordial antimatter and dark matter [28][29][30]. As it turns out, the low momentum characteristic yields of antinuclei at central rapidities (compared to forward) lie in an energy region which is best suited for identification by most satellite-borne (low magnetic-field) instruments, such as AMS-02 [28].…”
Section: Introductionmentioning
confidence: 99%
“…Big-bang nucleosynthesis is the dominant natural source of deuterons [27] and, in the absence of baryogenesis, one could assume that the same holds for antideuterons. These antinuclei and even heavier antinuclei can also be produced in pp and pA collisions in interstellar space, representing a background source in the searches for segregated primordial antimatter and dark matter [28][29][30]. As it turns out, the low momentum characteristic yields of antinuclei at central rapidities (compared to forward) lie in an energy region which is best suited for identification by most satellite-borne (low magnetic-field) instruments, such as AMS-02 [28].…”
Section: Introductionmentioning
confidence: 99%
“…Using the knowledge gained from the successful prototype GAPS flight [10] [11] and the Si(Li) detector development, work is now progressing towards optimizing the detector fabrication scheme for full flight detector production. The main milestones of this effort are: to verify Li drifting uniformity and build drifting stations capable of drifting 5-10 cm diameter wafers with minimal temperature variations; to either achieve similar high-yield, high-performance production of 10-cmdiameter Si(Li) detectors as demonstrated in 5-cm-diameter detectors, or to fallback to an existing design that utilizes 5cm-diameter detectors to yield the same sensitivity; to implement a scaled-up facility for batch processing of all flight detectors; and to develop ASICs, based on existing prototypes, as well as a final custom pre-amplifier for the Si(Li) detectors.…”
Section: Discussionmentioning
confidence: 99%
“…6). 12,13) The pGAPS OHP was developed on the basis of the scaled down U-shaped model described in the previous Section 2.2; it consists of 10 turns of U-shaped tubes each with a check valve, dummy heat load strips on the heating section, a white painted radiator attached to the cooling section, and an albedo shield attached to the adiabatic section. The reservoir was disconnected before the flight.…”
Section: Flight Demonstration With a Scaled-down Ohp Modelmentioning
confidence: 99%